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  • Other Sources  (306)
  • Man/System Technology and Life Support  (138)
  • Space Sciences (General)  (124)
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  • 1
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-33,21〈1900〉;KART H 140:Neuenburg
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 036 20 - E 036 30 / N 053 42 - N 053 36.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Nowe ; Neuenburg ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 126
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  • 2
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-25,43〈1921〉;KART H 140:Lüneburg
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 028 00 - E 028 10 / N 053 18 - N 053 12.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Lüneburg ; Geologische Karte ; GeoTIFF ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 66
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  • 3
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140 5203;KART H 140:Stolberg
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 023 50 - E 024 00 / N 050 48 - N 050 42.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Stolberg ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 92
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  • 4
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140 5204;KART H 140:Lendersdorf
    Publication Date: 2021-07-22
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 024 00 - E 024 10 / N 050 48 - N 050 42.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Geologische Karte ; Lendersdorf ; GeoTIFF ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 66
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  • 5
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140 5202;KART H 140:Aachen
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 023 40 - E 023 50 /N 050 48 - N 050 42.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Aachen ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 80
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  • 6
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:5103;KART H 140:Eschweiler
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Eschweiler ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 130
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  • 7
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-17,5〈1914〉;KART H 140:Rauschen
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro: E 037 40 - E 037 50 / N 055 00 - N 054 54.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Светлогорск ; GeoTIFF ; Rauschen ; Geologische Karte ; Swetlogorsk ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 164
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  • 8
    Publication Date: 2021-03-29
    Description: Die meisten Moore in Nordwestdeutschland werden seit mehreren Jahrhunderten landwirtschaftlich genutzt. Die Kultivierungsverfahren der Moore entscheiden, welche Nutzungen möglich sind. Tiefumbruchböden lassen sich vielfältig, überwiegend als Acker nutzen. Auf den Schwarzkulturen dominiert heute die standortgerechte Grünlandnutzung, wobei die nicht standortgerechte, ackerbauliche Nutzung in jüngster Zeit zugenommen hat. Mit zunehmender Intensität der Flächenbewirtschaftung verschlechtern sich die Torfeigenschaften und durch Mineralisierung der Torfe treten Höhenverluste auf. Die Grenzen der Befahrbarkeit bzw. Trittfestigkeit werden häufig erreicht. In der Nährstoffdynamik unterscheiden sich Hoch- und Niedermoore. Bei der extensiven Grünlandnutzung, verbunden mit reduzierter Entwässerungsintensität, bereiten häufig Flatterbinse (Juncus effusus) und Rasenschmiele (Deschampsia caespitosa) Probleme. Neue Nutzungsverfahren der Paludikultur befinden sich noch in der Entwicklung und Erprobung. Eine dauerhafte Sicherung der Produktionsstandorte für landwirtschaftliche Nutzungen ist auf Tiefumbruchböden möglich.
    Description: report
    Keywords: 553.21 ; Moor ; land-use ; Landwirtschaft ; peatland ; FID-GEO-DE-7
    Language: German
    Type: article , publishedVersion
    Format: 19
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  • 9
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:6307;KART H 140:Hermeskeil
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 024 30 - E 024 40 / N 049 42 - N 049 36.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Hermeskeil ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 26
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  • 10
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-14,31〈1897〉;KART H 140:Rügenwalde
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch die SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 034 00 - E 034 10 / N 054 30 - N 054 24.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Rügenwalde ; Geologische Karte ; Darłowo ; GeoTIFF ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 96
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  • 11
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    Kraatz, Berlin
    In:  Geologisches Institut, Leibniz Universität Hannover | SUB Göttingen | KART H 140:Hermannsburg
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat des Geologischen Instituts der Leibniz Universität Hannover. Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 027 40 - E 027 50 /N 052 54 - N 052 48.
    Description: map
    Description: Leibniz Universität Hannover/Geologisches Institut, DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Hermannsburg ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 70
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  • 12
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    Kraatz, Berlin
    In:  Geologisches Institut, Leibniz Universität Hannover | SUB Göttingen | -;KART H 140:Unterlüß
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat des Geologischen Instituts der Leibniz Universität Hannover. Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 027 50 - E 028 00 /N 052 54 - N 052 48.
    Description: map
    Description: Leibniz Universität Hannover/Geologisches Institut, DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Unterlüss ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 56
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  • 13
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-18,2〈1914〉;KART H 140:Bledau
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 038 10 - E 038 20 /N 055 00 - N 054 54.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Geologische Karte ; GeoTIFF ; Bledau ; Sosnowka ; Сосновка ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 134
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  • 14
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-18,7〈1914〉;KART H 140:Rudau
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 038 00 - E 038 10 /N 054 54 - N 054 48.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Rudau ; Melnikowo ; Мельниково ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 104
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  • 15
    Publication Date: 2021-03-29
    Description: Die Bedeutung der Moore als besondere Archive der Natur- und Kulturgeschichte wird beschrieben und im Hinblick auf die Entstehung und Entwicklung der Moorarchäologie in Niedersachsen diskutiert. Unter Einbeziehung der Beschreibung heute in der Moorarchäologie zum Einsatz kommender Arbeitsverfahren, werden die Bedeutung der Moore als Bestandteil früher Lebewelten und sozio-kultureller Prozesse beleuchtet. Abschließend werden die gesetzlichen Möglichkeiten zum Schutz des archäologischen Erbes im Moor aufgezeigt.
    Description: report
    Keywords: 553.21 ; Moor ; Archäologie ; FID-GEO-DE-7
    Language: German
    Type: article , publishedVersion
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  • 16
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-18,8〈1914〉;KART H 140:Powunden
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 038 10 - E 038 20 /N 054 54 - N 054 48.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Geologische Karte ; Powunden ; Chrabrowo ; Храброво ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 112
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  • 17
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-17,11〈1914〉;KART H 140:Germau
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 037 40 - E 037 50 /N 054 54 - N 054 48.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Germau ; Russkoje ; Русское ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 140
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  • 18
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-17,4〈1914〉;KART H 140:Gr.-Dirschkeim
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 037 30 - E 037 40 /N 055 00 - N 054 54
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Gr. Dirschkeim ; Donskoje ; Донское ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 162
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  • 19
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-17,10〈1914〉;KART H 140:Palmnicken
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 037 30 - E 037 40 /N 054 54 - N 054 48.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Palmnicken ; Jantarny ; Янтарный ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 118
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  • 20
    Publication Date: 2021-03-29
    Description: Subfossile Kiefern werden in vielen Mooren Nordwestdeutschlands gefunden. Durch die Transgression der Moore wurden Kiefern an der Basis der Torfe eingebettet und befinden sich oft am Übergang von Niedermoor- zu Hochmoortorfen. Stubbenhorizonte innerhalb der Torfkörper dokumentieren Bewaldungsphasen der Moore. Durch dendrochronologische Untersuchungen wurden subfossile Kiefern von 40 Fundorten datiert und erstmalig eine Kiefernchronologie für Nordwestdeutschland aufgebaut. Die untersuchten Kiefernhölzer belegen zu bestimmten Zeitabschnitten gehäufte Absterbe- oder Keimungsphasen sowie signifikante Änderungen der Jahrringbreiten der Hölzer aus verschiedenen Mooren. Teilweise zeichnen sich auch bei den früher bearbeiteten subfossilen Eichen zeitparallel entsprechende Phasen ab, so dass diese Signale, klimatisch verursacht, als Abbild von Vernässungsphasen angesehen werden.
    Description: research
    Keywords: 553.21 ; Moor ; Dendroökologie ; Dendrochronologie ; Pinus ; FID-GEO-DE-7
    Language: German
    Type: article , publishedVersion
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  • 21
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    Kraatz, Berlin
    In:  Geologisches Institut, Leibniz Universität Hannover | SUB Göttingen | KART H 140:Lüneburg
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat des Geologischen Instituts der Leibniz Universität Hannover. Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 028 00 - E 028 10 / N 053 18 - N 053 12.
    Description: map
    Description: Leibniz Universität Hannover/Geologisches Institut, DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Lüneburg ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 66
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  • 22
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-17,12〈1914〉;KART H 140:Pobethen
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 037 50 - E 038 00 /N 054 54 - N 054 48.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Pobethen ; Romanowo ; Романово ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 108
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  • 23
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:6208;KART H 140:Morscheid
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 024 40 – 024 50 / N 049 48 - 049 42.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Morscheid ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 30
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  • 24
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:6209;KART H 140:Oberstein
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 024 50 – E 025 00 / N 049 48 - N 049 42.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Oberstein ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 66
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:6308;KART H 140:Buhlenberg
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 024 40 – E 024 50 / N 049 42 - N 049 36.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Geologische Karte ; Buhlenberg ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 50
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:5527;KART H 140:Ostheim
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 027 50 – E 028 00 / N 050 30 – N 050 24.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Ostheim v. d. Rhön ; Mellrichstadt ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 58
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:5525;KART H 140:Gersfeld
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 027 30 – E 027 40 / N 050 30 – N 050 24.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Geologische Karte ; Gersfeld ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 48
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-17,6〈1914〉;KART H 140:Neukuhren
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 037 50 - E 038 00 /N 055 00 - N 054 54.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Neukuhren ; Pionerski ; Пионерский ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 126
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-14,39〈1897〉;KART H 140:Schlawe
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 034 20 - E 034 30 / N 054 24 - N 054 18.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Sławno ; Schlawe ; Geologische Karte ; GeoTIFF ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 110
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | Kart. W 15710-57,39〈1874〉
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000. Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Koordinaten Vorlage: Nullmeridian Ferro E 029 - 030 / N 051 – 052.
    Description: map
    Description: Staatsbibliothek Berlin (SBB)
    Keywords: 912 ; 554.3 ; Schafstädt ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 1
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  • 31
    Publication Date: 2021-03-29
    Description: We focus on new gravity and gravity gradient data sets from modern satellite missions GOCE, GRACE and CHAMP, and their geophysical interpretation at passive continental margins of the South Atlantic. Both sides, South Africa and South America, have been targets of hydrocarbon exploration and academic research of the German Priority Program SAMPLE (South Atlantic Margin Processes and Links with onshore Evolution). The achievable spatial resolution, driven by GOCE, is 70–80 km. Therefore, most of the geological structures, which cause a significant gravity effect (by both size and density contrast), can be resolved. However, one of the most important aspects is the evaluation of the omission error, which is not always in the focus of interpreters. It results from high-frequency signals of very rough topographic and bathymetric structures, which cannot be resolved by satellite gravimetry due to the exponential signal attenuation with altitude. The omission error is estimated from the difference of the combined gravity model EIGEN-6C4 and the satellite-only model GOCO05S. It can be significantly reduced by topographic reductions. Simple 2D density models and their related mathematical formulas provide insights in the magnitude of the gravity effect of masses that form a passive continental margin. They are contrasted with results from satellite-only and combined gravity models. Example geophysical interpretations are given for the western and eastern margin of the South Atlantic Ocean, where standard deviations vary from 25 to 16 mGal and 21–11 mGal, respectively. It could be demonstrated, that modern satellite gravity data provide significant added value in the geophysical gravity data processing domain and in the validation of heterogeneous terrestrial data bases. Combined models derived from high-resolution terrestrial gravity and homogeneous satellite data will lead to more detailed and better constrained lithospheric density models, and hence will improve our knowledge about structure, evolution and state of stress in the lithosphere.
    Description: DFG
    Description: research
    Keywords: 551.1 ; 550.28 ; 550 ; TQI 000 ; Satelliten-Geophysik ; Combination of terrestrial and satellite gravity ; Satellite gravity and gradients ; 2nd derivation of satellite gravity ; FID-GEO-DE-7
    Language: English
    Type: article , publishedVersion
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:5102;KART H 140:Herzogenrath
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 023 40 - E 023 50 / N 050 54 - N 050 48.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Geologische Karte ; Herzogenrath ; GeoTIFF ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 86
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    Kraatz, Berlin
    In:  SUB Göttingen | KART B 140:5104;KART H 140:Düren
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), Karte aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 024 00 - E 024 10 / N 050 54 - N 050 48.
    Description: map
    Description: DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Geologische Karte ; Düren ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 92
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-18,1〈1914〉;KART H 140:Kranz
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. GeoTIFF erstellt durch FID GEO, SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 038 00 - E 038 10 /N 055 00 - N 054 54.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Geologische Karte ; GeoTIFF ; Cranz ; Selenogradsk ; Зеленоградск ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 110
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-33,22〈1900〉;KART H 140:Garnsee
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 036 30 - E 036 40 / N 053 42 - N 053 36.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Gardeja ; Garnsee ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 128
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-33,16〈1882〉;KART H 140:Marienwerder
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 036 30 - E 036 40 / N 053 48 - N 053 42.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Marienwerder ; Kwidzyn ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 144
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-33,15〈1889〉;KART H 140:Münsterwalde
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. koordinaten Vorlage: Nullmeridian Ferro E 036 20 - E 036 30 / N 053 48 - N 053 42.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Opalenie ; Münsterwalde ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 110
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    Kraatz, Berlin
    In:  Staatsbibliothek Berlin (SBB) | SUB Göttingen | Kart. W 15710-33,29〈1898〉;KART H 140:Lessen
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat der Staatsbibliothek Berlin (SBB), bereitgestellt durch den Fachinformationsdienst Kartographie und Geobasisdaten (FID Karten). Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 036 40 - E 036 50 / N 053 36 - N 053 30.
    Description: map
    Description: Staatsbibliothek Berlin (SBB), DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; Łasin ; Lessen ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 102
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    Kraatz, Berlin
    In:  Geologisches Institut, Leibniz Universität Hannover | SUB Göttingen | KART H 140:Celle
    Publication Date: 2021-06-02
    Description: Geologische Karte 1: 25 000 mit Erläuterungen. Die Karte ist ein Digitalisat des Geologischen Instituts der Leibniz Universität Hannover. Das Erläuterungsheft ist ein Digitalisat des FID GEO (Fachinformationsdienst Geowissenschaften der festen Erde), erstellt durch das GDZ (Göttinger Digitalisierungszentrum), aus dem Bestand der SUB Göttingen. Koordinaten Vorlage: Nullmeridian Ferro E 027 40 - E 027 50 /N 052 42 - N 052 36.
    Description: map
    Description: Leibniz Universität Hannover/Geologisches Institut, DFG, SUB Göttingen
    Keywords: 912 ; 554.3 ; GeoTIFF ; Celle ; Geologische Karte ; FID-GEO-DE-7
    Language: German
    Type: map_digi
    Format: 74
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    Geounion Alfred-Wegener-Stiftung, Berlin
    In:  Herausgeberexemplar
    Publication Date: 2021-08-30
    Description: This volume contains the program, abstracts and field guides of the centenary meeting of the Paläontologische Gesellschaft (September 2012, Berlin). The topics of the symposia are: •The Alfred Wegener Centennial Symposium: The Idea that Changed the World – 100 Years of Continental Drift •Biodiversity in the Fossil Record – Going Beyond How Many Taxa •Frontiers in Geobiology •Stories from the Past – Reading Biomineralized Diaries •New Challenges in Micropalaeontology – Going Beyond the Standards •Evolution, Development, and Developmental Paleontology – the Interplay of Ontogenetic and Deep Time •Anomalies and Pathologies – the Other Sources of Variation •Taphonomy – Preservation of Ecological and Biogeographic Attributes in the Sedimentary Record •Bridging the Gap – Cross-Discipline Research in Biology and Palaeontology •The Cambrian Bioradiation of Metazoa – an Interdisciplinary Approach •Climate Change and Biodiversity Patterns in the Mid-Paleozoic (IGCP 596) •The Triassic – Organismic Evolution Between Two Mass Extinction Events •The Early Evolution of Tetrapods and their Ecosystems •Tendaguru and Beyond – Vertebrates in Jurassic Terrestrial Ecosystems •Biological Factors of Sauropod Gigantism •Mammalian Dentitions – Diversity, Form, and Function •Amber as a Window to Terrestrial Palaeoecosystems •More than just Wet Feet – Tetrapod Transitions from Land to Sea and Hot Spots of Marine Tetrapod Evolution •The Evolution of Modern African Biogeography •Gymnosperm Evolution – Major Events and Mysteries •The Development of Modern Vegetation Belts During the Cretaceous and Tertiary •Öffentlichkeitsarbeit – Vernetzung oder Abgrenzung? •The Young Palaeontologist Award •Open Symposia •Tilly-Edinger Award
    Description: conference
    Keywords: 560 ; Paläontologie ; Paläontologische Gesellschaft ; Paläontologie ; Kongress ; Berlin 2012 ; paleontology ; FID-GEO-DE-7
    Language: English
    Type: anthology , publishedVersion
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    GeoUnion, Berlin
    In:  Herausgeberexemplar
    Publication Date: 2021-08-30
    Description: During the past years there has been a great amount of new publications on varved sediment records, some of them describing methodological developments and others forming a basis of interpretation of climate and environmental change of mainly postglacial times. In many studies, the varve chronologies of lacustrine and marine sediments form a solid basis of dating, not to mention the environmental and climate signal that is stored in varves and laminae they contain. Since two years a step forward has been taken and the varve community is gathering during annual Varves Working Group (VWG) workshops to summarize what has been accomplished during the past decade and to exchange new ideas and promote their use in global climate reconstructions. The VWG has formed under the frame of the PAGES cross cutting theme 1 (CCT1) “Chronology” and CCT2 “Proxy development, calibration, validation” to address a number of topics with workshops and products. The main topics of the VWG include: •Methodological developments •Marine versus lacustrine varves •Varve chronologies, including quantification of age uncertainties •Calibration of archived climatic and environmental signals •Database management •Data processing •Learning from other annually resolved archives.
    Description: conference
    Keywords: 551 ; Rhythmite {Sedimentologie} ; Warvenmethoden ; Instrumentelle Ergebnisse zu Klimaänderungen und Klimaschwankungen ; Warve ; Rhythmit ; Warvenchronologie ; Kongress ; Manderscheid 2012 ; varve ; FID-GEO-DE-7
    Language: English
    Type: anthology , publishedVersion
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    GeoUnion Alfred-Wegener-Stifung, Berlin
    In:  Herausgeberexemplar
    Publication Date: 2021-08-30
    Description: This 4th International PASADO Workshop is related to the research initiative “Potrok Aike Lake Sediment Archive Drilling Project” (PASADO) within the framework of the “International Continental Scientific Drilling Programme” (ICDP). PASADO addresses challenging issues of geoscientific and socioeconomic relevance related to Earth history and climate like qualitative and quantitative climatic and environmental reconstruction as well as reconstruction of the palaeosecular variation of the Earth's magnetic field but also natural hazards like fire history, frequency of volcanic activity including tephra fallout and dust deposition. The history of volcanic activities for the last ca. 50,000 years is another interesting topic. Moreover, dust and tephra records provide links of this unique southern hemispheric terrestrial record to marine sediment archives and to ice cores from Antarctica. Finally, obtained reconstructions of climate variability will be compared statistically with the output of Global Circulation Model (GCM) simulations to improve our understanding of forcing mechanisms of the global climate.
    Description: conference
    Keywords: 551 ; Geologische Bohrungen in einzelnen Regionen ; Argentinien {Geologie} ; Sedimente bestimmter Regionen ; Paläolimnologie {Geologie} ; Argentina ; sediments ; palaeoclimate ; palaeoenvironment ; tephra ; volcanism ; FID-GEO-DE-7
    Language: English
    Type: anthology , publishedVersion
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    GeoUnion Alfred-Wegener-Stifung, Berlin
    In:  Herausgeberexemplar
    Publication Date: 2021-08-30
    Description: The understanding of early agrarian economies and their impact on landscapes and natural environments has become a major goal of many large-scale projects. The shaping of cultural landscapes by the spread of agriculture, animal husbandry and the building of settlements has been the most influential development since the beginning of agriculture more than 10.000 years ago. Sessions: •Gathering, Cultivation and Domestication •Ethnobotanical approaches •Methods and Analytical Archaeobotany •Regional and Historical Archaeobotany •Origins of agriculture in the Near East.
    Description: conference
    Keywords: 561 ; Palaeophytogeographie {Paläobotanik} ; Holozän {Paläobotanik} ; Ethnobotanik. Ethnozoologie {Ethnologie} ; Paläoethnobotanik ; Archäobotanik ; Kongress ; archaeobotany ; palaeoethnobotany ; agriculture ; palaeoenvironment ; Holocene ; human impact ; FID-GEO-DE-7
    Language: English
    Type: anthology , publishedVersion
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    GeoUnion Alfred-Wegener-Stifung, Berlin
    In:  Herausgeberexemplar
    Publication Date: 2021-08-30
    Description: This 2nd International PASADO Workshop is based on the research initiative “Potrok Aike Lake Sediment Archive Drilling Project” (PASADO) within the framework of the “International Continental Scientific Drilling Programme” (ICDP). PASADO addresses several challenging issues of geoscientific and socioeconomic relevance related to Earth history and climate like qualitative and quantitative climatic and environmental reconstruction as well as reconstruction of the palaeosecular variation of the Earth's magnetic field and natural hazards like fire history, frequency of volcanic activity including tephra fallout or dust deposition. The history of volcanic activities for the last ca. 50,000 years is another interesting topic. Moreover, dust and tephra records will provide means to link this unique southern hemispheric terrestrial record to marine sediment archives and to ice cores from Antarctica. Finally, obtained reconstructions of climate variability will be compared statistically with the output of Global Circulation Model (GCM) simulations to improve our understanding of forcing mechanisms of the global climate.
    Description: conference
    Keywords: 551 ; Geologische Bohrungen in einzelnen Regionen ; Argentinien {Geologie} ; Sedimente bestimmter Regionen ; sediments ; Argentina ; palaeoenvironment ; palaeoclimate ; tephra ; volcanism ; FID-GEO-DE-7
    Language: English
    Type: anthology , publishedVersion
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  • 45
    Publication Date: 2019-07-19
    Description: Human missions to Mars may require radical changes in the approach to extra-vehicular (EVA) suit design. A major challenge is the balance of building a suit robust enough to complete multiple EVAs under intense ultraviolet (UV) light exposure without losing mechanical strength or compromising the suit's mobility. To study how the materials degrade on Mars in-situ, the Jet Propulsion Laboratory (JPL) invited the Advanced Space Suit team at NASA's Johnson Space Center (JSC) to place space suit materials on the Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals (SHERLOC) instrument's calibration target of the Mars 2020 rover. In order to select materials for the rover and understand the effects from Mars equivalent UV exposure, JSC conducted ground testing on both current and new space suit materials when exposed to 2500 hours of Mars mission equivalent UV. To complete this testing, JSC partnered with NASA's Marshall Space Flight Center to utilize their UV vacuum chambers. Materials tested were Orthofabric, polycarbonate, Teflon, Dacron, Vectran, spectra, bladder, nGimat coated Teflon, and nGimat coated Orthofabric. All samples were measured for mass, tensile strength, and chemical composition before and after radiation. Mass loss was insignificant (less than 0.5%) among the materials. Most materials loss tensile strength after radiation and became more brittle with a loss of elongation. Changes in chemical composition were seen in all radiated materials through Spectral Analysis. Results from this testing helped select the materials that will fly on the Mars 2020 rover. In addition, JSC can use this data to create a correlation to the chemical changes after radiation-which is what the rover will send back while on Mars-to the mechanical changes, such as tensile strength.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-37805 , International Conference on Environmental Systems (ICES 2017); Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
    Format: application/pdf
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  • 46
    Publication Date: 2019-07-19
    Description: NASA has established the goal of traveling beyond low-Earth orbit and extending manned exploration to Mars. The length of proposed Mars missions and the lack of resupply missions increases the importance of nutritional content in the food system, which will need a five-year shelf life. The purpose of this research is to assess the stability of vitamin supplementation in traditionally processed spaceflight foods. It is expected that commercially available fortification nutrients will remain stable through a long duration exploration mission at sufficient levels if compatible formulation, processing, and storage temperatures are achieved. Five vitamins (vitamin E, vitamin K, pantothenic acid, folic acid, and thiamin) were blended into a vitamin premix (DSM, Freeport, TX) such that the vitamin concentration per serving equaled 25% of the recommended daily intake after two years of ambient storage. Four freeze-dried foods (Scrambled Eggs, Italian Vegetables, Potatoes Au Gratin, Noodles and Chicken) and four thermo-stabilized foods (Curry Sauce with Vegetables, Chicken Noodle Soup, Grilled Pork Chop, Rice with Butter) were produced, with and without the vitamin premix, to assess the impact of the added fortification on color and taste and to determine the stability of supplemental vitamins in spaceflight foods. The addition of fortification to spaceflight foods did not greatly alter the organoleptic properties of most products. In most cases, overall acceptability scores remained above 6.0 (minimum acceptable score) following six months and one year of low-temperature storage. Likewise, the color of fortified products appears to be preserved over one year of storage. The only exceptions were Grilled pork Chop and Chicken Noodle Soup whose individual components appeareddegrade rapidly over one year of storage. Finally, most vitamins appeared to be stable during long-term storage. The only exception was thiamin, which degraded rapidly during the first year of storage at 35C. It was previously believed that the imprecise method of fortification would prove problematic for nutrient quantification; however, this was only an issue in stored samples of Grilled Pork Chop, Italian Vegetables and Curry Sauce with Vegetables. Year two data may further reveal the extent to which this is a problem, as well as identify overall quality changes over time.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-37794 , NASA HRP Investigators'' Workshop; Jan 23, 2017 - Jan 26, 2017; Galveston, TX; United States
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  • 47
    Publication Date: 2019-07-19
    Description: This paper continues the annual tradition of summarizing at this conference the results of chemical analyses performed on archival potable water samples returned from the International Space Station (ISS). 2016 represented a banner year for life on board the ISS, including the successful conclusion for two crew members of a record one-year mission. Water reclaimed from urine and/or humidity condensate remained the primary source of potable water for the crew members of ISS Expeditions 46-50. The year 2016 was also marked by the end of a long-standing tradition of U.S. sampling and monitoring of Russian Segment potable water sources. Two water samples taken during Expedition 46 in February 2016 and returned on Soyuz 44, represented the final Russian Segment samples to be collected and analyzed by the U.S. side. Although anticipated for 2016, a rise in the total organic carbon (TOC) concentration of the product water from the U.S. water processor assembly due to breakthrough of organic contaminants from the system did not materialize, as evidenced by the onboard TOC analyzer and archive sample results.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-37969 , International Conference on Environmental Systems; Apr 16, 2017 - Apr 20, 2017; Charleston, SC; United States
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  • 48
    Publication Date: 2019-07-12
    Description: Multiple organizations within NASA as well as industry and academia fund and participate in research related to extravehicular activity (EVA). In October 2015, representatives of the EVA Office, the Crew and Thermal Systems Division (CTSD), and the Human Research Program (HRP) at NASA Johnson Space Center agreed on a formal framework to improve multi-year coordination and collaboration in EVA research. At the core of the framework is an Integrated EVA Human Research Plan and a process by which it will be annually reviewed and updated. The over-arching objective of the collaborative framework is to conduct multi-disciplinary cost-effective research that will enable humans to perform EVAs safely, effectively, comfortably, and efficiently, as needed to enable and enhance human space exploration missions. Research activities must be defined, prioritized, planned and executed to comprehensively address the right questions, avoid duplication, leverage other complementary activities where possible, and ultimately provide actionable evidence-based results in time to inform subsequent tests, developments and/or research activities. Representation of all appropriate stakeholders in the definition, prioritization, planning and execution of research activities is essential to accomplishing the over-arching objective. A formal review of the Integrated EVA Human Research Plan will be conducted annually. Coordination with stakeholders outside of the EVA Office, CTSD, and HRP is already in effect on a study-by-study basis; closer coordination on multi-year planning with other EVA stakeholders including academia is being actively pursued. Details of the preliminary Integrated EVA Human Research Plan are presented including description of ongoing and planned research activities in the areas of: physiological and performance capabilities; suit design parameters; EVA human health and performance modeling; EVA tasks and concepts of operations; EVA informatics; human-suit sensors; suit sizing and fit; and EVA injury risk and mitigation. This paper represents the 2017 update to the Integrated EVA Human Research Plan.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-38643
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  • 49
    Publication Date: 2019-07-12
    Description: The Environmental Control System provides a controlled air purge to Orion and SLS. The ECS performs this function by processing 100% ambient air while simultaneously controlling temperature, pressure, humidity, cleanliness and purge distribution.
    Keywords: Man/System Technology and Life Support
    Type: KSC-E-DAA-TN43751
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  • 50
    Publication Date: 2019-07-12
    Description: No abstract available
    Keywords: Space Sciences (General)
    Type: MSFC-E-DAA-TN40559
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  • 51
    Publication Date: 2019-07-12
    Description: No abstract available
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-38351
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  • 52
    Publication Date: 2019-07-12
    Description: Electrochemical and crevice corrosion laboratory test results are presented for three noble metal candidates with possible application on the Universal Waste Management System (UWMS) in support of the Environmental Control and Life Support System (ECLSS) aboard the International Space Station (ISS). The three metal candidates, which included Inconel 625, Hastelloy C276 and Titanium 6Al-4V, were evaluated in two solutions representative of the acidic pretreatment formulations utilized during processing of waste liquids within the ECLSS. Final test results and data analysis indicated that the passive layer on all three metals provides excellent corrosion protection in both solutions under standard test conditions.
    Keywords: Man/System Technology and Life Support
    Type: NASA/CR-2017-218240 , M-1432
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  • 53
    Publication Date: 2019-07-12
    Description: Contamination of a crewed spacecraft's cabin environment leading to environmental control and life support system (ECLSS) functional capability and operational margin degradation or loss can have an adverse effect on NASA's space exploration mission figures of merit-safety, mission success, effectiveness, and affordability. The role of evaluating the ECLSS's compatibility and cabin environmental impact as a key component of pass trace contaminant control is presented and the technical approach is described in the context of implementing NASA's safety and mission success objectives. Assessment examples are presented for a variety of chemicals used in vehicle systems and experiment hardware for the International Space Station program. The ECLSS compatibility and cabin environmental impact assessment approach, which can be applied to any crewed spacecraft development and operational effort, can provide guidance to crewed spacecraft system and payload developers relative to design criteria assigned ECLSS compatibility and cabin environmental impact ratings can be used by payload and system developers as criteria for ensuring adequate physical and operational containment. In additional to serving as an aid for guiding containment design, the assessments can guide flight rule and procedure development toward protecting the ECLSS as well as approaches for contamination event remediation.
    Keywords: Man/System Technology and Life Support
    Type: NASA/TP-2017-219846 , M-1449
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  • 54
    Publication Date: 2019-07-12
    Description: NASA's Human Research Program (HRP) funds research efforts aimed at mitigating various human health and performance risks, including the Risk of Inadequate Design of Human and Automation/Robotic Integration (HARI). As such, within HRP, the Human Factors and Behavioral Performance (HFBP) Element tasked an evaluation of future HARI needs in order to scope and focus the HARI risk research plan. The objective was to provide a systematic understanding of the critical factors associated with effective HARI that will be necessary to achieve the future mission goals for near- and deep-space exploration. Future mission goals are specified by NASA Design Reference Missions (DRMs) that are pertinent to the HRP. The outcome of this evaluation is a set of NASA-relevant HARI tasks, factors, and interactions required for exploration-class missions.
    Keywords: Man/System Technology and Life Support
    Type: NASA/TM-2017-219516 , ARC-E-DAA-TN40802
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  • 55
    Publication Date: 2019-07-19
    Description: Spectra or similar Ultra-high-molecular-weight polyethylene (UHMWPE) fabric is the likely choice for future structural space suit restraint materials due to its high strength-to-weight ratio, abrasion resistance, and dimensional stability. During long duration space missions, space suits will be subjected to significant amounts of high-energy radiation from several different sources. To insure that pressure garment designs properly account for effects of radiation, it is important to characterize the mechanical changes to structural materials after they have been irradiated. White Sands Test Facility (WSFTF) collaborated with the Crew and Thermal Systems Division at the Johnson Space Center (JSC) to irradiate and test various space suit materials by examining their tensile properties through blunt probe puncture testing and single fiber tensile testing after the materials had been dosed at various levels of simulated GCR and SPE Iron and Proton beams at Brookhaven National Laboratories. The dosages were chosen based on a simulation developed by the Structural Engineering Division at JSC for the expected radiation dosages seen by space suit softgoods seen on a Mars reference mission. Spectra fabric tested in the effort saw equivalent dosages at 2x, 10x, and 20x the predicted dose as well as a simulated 50 year exposure to examine the range of effects on the material and examine whether any degradation due to GCR would be present if the suit softgoods were stored in deep space for a long period of time. This paper presents the results of this work and outlines the impact on space suit pressure garment design for long duration deep space missions.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-37904 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 56
    Publication Date: 2019-07-19
    Description: For the past four years, the Air Quality Monitor (AQM) has been the operational instrument for measuring trace volatile organic compounds on the International Space Station (ISS). The key components of the AQM are the inlet preconcentrator, the gas chromatograph (GC), and the differential mobility spectrometer. Most importantly, the AQM operates at atmospheric pressure and uses air as the GC carrier gas, which translates into a small reliable instrument. Onboard ISS there are two AQMs, with different GC columns that detect and quantify 22 compounds. The AQM data contributes valuable information to the assessment of air quality aboard ISS for each crew increment. The U.S. Navy is looking to update its submarine air monitoring suite of instruments, and the success of the AQM on ISS has led to a jointly planned submarine sea trial of a NASA AQM. In addition to the AQM, the Navy is also interested in the Multi-Gas Monitor (MGM), which was successfully flown on ISS as a technology demonstration to measure major constituent gases (oxygen, carbon dioxide, water vapor, and ammonia). A separate paper will present the MGM sea trial results. A prototype AQM, which is virtually identical to the operational AQM, has been readied for the sea trial. Only one AQM will be deployed during the sea trial, but it is sufficient to detect the compounds of interest to the Navy for the purposes of this trial. A significant benefit of the AQM is that runs can be scripted for pre-determined intervals and no crew intervention is required. The data from the sea trial will be compared to archival samples collected prior to and during the trial period. This paper will give a brief overview of the AQM technology and protocols for the submarine trial. After a quick review of the AQM preparation, the main focus of the paper will be on the results of the submarine trial. Of particular interest will be the comparison of the contaminants found in the ISS and submarine atmospheres, as both represent closed environments. In U.K. submarine trials in the early 2000s, the submarine and ISS atmospheres were found to be remarkably similar.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-37932 , International Conference on Environmental Systems (ICES); Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 57
    Publication Date: 2019-07-19
    Description: For many years, the NASA Orbital Debris Program Office has been collecting measurements of the orbital debris environment from the Haystack Ultra-wideband Satellite Imaging Radar (HUSIR) and its auxiliary (HAX). These measurements sample the small debris population in low earth orbit (LEO). This paper will provide an overview of recent observations and highlight trends in selected debris populations. Using the NASA size estimation model, objects with a characteristic size of 1 cm and larger observed from HUSIR will be presented. Also, objects with a characteristic size of 2 cm and larger observed from HAX will be presented.
    Keywords: Space Sciences (General)
    Type: JSC-CN-38191 , European Conference on Space Debris; Apr 18, 2017 - Apr 21, 2017; Darmstadt; Germany
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  • 58
    Publication Date: 2019-07-20
    Description: The development of a microgravity air-evaporation urine brine dryer (CapiBRiC - Capillary Brine Residual in Containment) that releases its effluent gas into the cabin of the International Space Station will require some form of a demister to guarantee that no acid, chromium, or other hazardous materials are released within the effluent gas stream. A hydrophobic membrane demister can be used for this application, and can be compatible with the proposed high flow rates of the effluent gas stream. This paper will describe the construction and sizing of such a membrane demister.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-62 , ARC-E-DAA-TN39524 , International Conference on Environmental Systems (ICES 2017); Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 59
    Publication Date: 2019-07-13
    Description: A laboratory investigation of acetone, an interstellar and cometary molecule, has produced new results concerning its decomposition in a radiation environment. Mid-infrared spectroscopy has been used to follow amorphous acetone's destruction by ionizing radiation (1 MeV protons) at 20 K. Radiation products identified are the CH4, CO, and CO2 usually made in such experiments, along with ketene, allene, and the acetonyl radical, all identified here for the first time in irradiated solid acetone. Evidence for the reduction product 2-propanol was suggestive, but a firm identification could not be made either for it or for the C2 hydrocarbons (i.e., C2H6, C2H4, C2H2). The acetyl radical was not observed as a radiation product. Isotopically labeled reagents were used to demonstrate ketene formation and to emphasize that multiple approaches are needed for robust assignments of infrared spectral features of irradiated icy solids. Results from a supporting radiation experiment with isotopically labeled acetic acid are described. Comparisons are made to a previous study of acetone's stability in extraterrestrial radiation environments, and caution is urged in measuring and interpreting CO abundances in irradiated icy solids.
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN56719 , Physical Chemistry Chemical Physics (ISSN 1463-9076) (e-ISSN 1463-9084); 8; 8; 5389-5398
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  • 60
    Publication Date: 2019-07-13
    Description: In the past decade thousands of exoplanet candidates and hundreds of confirmed exoplanets have been found. For sub-Neptune-sized planets, those less than approx. 10 Earth masses, we can separate planets into two broad categories: predominantly rocky planets, and gaseous planets with thick volatile sheaths. Observations and subsequent analysis of these planets show that rocky planets are only found with radii less than approx. 1.6 Earth radii. No rocky planet has yet been found that violates this limit. We propose that hydrodynamic escape of hydrogen rich protoatmospheres, accreted by forming planets, explains the limit in rocky planet size. Following the hydrodynamic escape model employed by Luger et al. (2015), we modelled the XUV driven escape from young planets (less than approx.100 Myr in age) around a Sun-like star. With a simple, first-order model we found that the rocky planet radii limit occurs consistently at approx. 1.6 Earth radii across a wide range of plausible parameter spaces. Our model shows that hydrodynamic escape can explain the observed cutoff between rocky and gaseous planets. Fig. 1 shows the results of our model for rocky planets between 0.5 and 10 Earth masses that accrete 3 wt. % H2/He during formation. The simulation was run for 100 Myr, after that time the XUV flux drops off exponentially and hydrodynamic escape drops with it. A cutoff between rocky planets and gaseous ones is clearly seen at approx. 1.5-1.6 Earth radii. We are only interested in the upper size limit for rocky planets. As such, we assumed pure hydrogen atmospheres and the highest possible isothermal atmospheric temperatures, which will produce an upper limit on the hydrodynamic loss rate. Previous work shows that a reasonable approximation for an upper temperature limit in a hydrogen rich protoatmosphere is 2000-3000 K, consistent with our assumptions. From these results, we propose that the observed dichotomy between mini-Neptunes and rocky worlds is simply explained by an early episode of thermally-driven hydrodynamic escape when host stars have saturated XUV fluxes.
    Keywords: Space Sciences (General)
    Type: ARC-E-DAA-TN42111 , Astrobiology Science Conference (AbSciCon 2017); Apr 24, 2017 - Apr 28, 2017; Mesa, AZ; United States
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  • 61
    Publication Date: 2019-07-13
    Description: Early Earth may have hosted a biologically mediated global organic haze during the Archean eon (3.8-2.5 billion years ago). This haze would have significantly impacted multiple aspects of our planet, including its potential for habitability and its spectral appearance. Here, we model worlds with Archean-like levels of carbon dioxide orbiting the ancient Sun and anM4Vdwarf (GJ 876) and show that organic haze formation requires methane fluxes consistent with estimated Earth-like biological production rates. On planets with high fluxes of biogenic organic sulfur gases (CS2, OCS, CH3SH, and CH3SCH3), photochemistry involving these gases can drive haze formation at lower CH4/CO2 ratios than methane photochemistry alone. For a planet orbiting the Sun, at 30x the modern organic sulfur gas flux, haze forms at a CH4/CO2 ratio 20% lower than at 1x the modern organic sulfur flux. For a planet orbiting the M4V star, the impact of organic sulfur gases is more pronounced: at 1x the modern Earth organic sulfur flux, a substantial haze forms at CH4/CO2 approx. 0.2, but at 30x the organic sulfur flux, the CH4/CO2 ratio needed to form haze decreases by a full order of magnitude. Detection of haze at an anomalously low CH4/ CO2 ratio could suggest the influence of these biogenic sulfur gases and therefore imply biological activity on an exoplanet. When these organic sulfur gases are not readily detectable in the spectrum of an Earth-like exoplanet, the thick organic haze they can help produce creates a very strong absorption feature at UV-blue wavelengths detectable in reflected light at a spectral resolution as low as 10. In direct imaging, constraining CH4 and CO2 concentrations will require higher spectral resolution, and R 〉 170 is needed to accurately resolve the structure of the CO2 feature at 1.57 microns, likely the most accessible CO2 feature on an Archean-like exoplanet.
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN50416 , Astrobiology (ISSN 1531-1074) (e-ISSN 1557-8070); 18; 4; 1666
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  • 62
    Publication Date: 2019-07-13
    Description: We present a path forward on a long-standing issue concerning the flux of small and slow meteoroids, which are believed to be the dominant portion of the incoming meteoric mass flux into the Earth's atmosphere. Such a flux, which is predicted by dynamical dust models of the Zodiacal Cloud, is not evident in ground-based radar observations. For decades this was attributed to the fact that the radars used for meteor observations lack the sensitivity to detect this population, due to the small amount of ionization produced by slow-velocity meteors. Such a hypothesis has been challenged by the introduction of meteor head echo (HE) observations with High Power and Large Aperture radars, in particular the Arecibo 430 MHz radar. Janches et al. developed a probabilistic approach to estimate the detectability of meteors by these radars and initially showed that, with the current knowledge of ablation and ionization, such particles should dominate the detected rates by one to two orders of magnitude compared to the actual observations. In this paper, we include results in our model from recently published laboratory measurements, which showed that (1) the ablation of Na is less intense covering a wider altitude range; and (2) the ionization probability, Beta ip, for Na atoms in the air is up to two orders of magnitude smaller for low speeds than originally believed. By applying these results and using a somewhat smaller size of the HE radar target we offer a solution that reconciles these observations with model predictions.
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN50883 , The Astrophysical Journal (ISSN 0004-637X) (e-ISSN 1538-4357); 843; 1; 1
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  • 63
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    In:  CASI
    Publication Date: 2019-07-13
    Description: A presentation of the current plan for the development of an exploration space suit pressure garment, beginning with a demonstration unit for the performance of EVA's on the ISS.
    Keywords: Man/System Technology and Life Support
    Type: JSC-E-DAA-TN49965 , Joint EVA Working Group Technical Interchange Meeting; Dec 06, 2017; Houston, TX; United States
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  • 64
    Publication Date: 2019-07-13
    Description: Challenges in retrieving D- and E-region Ne from GPS-RO, New algorithm, Initial results, Implications for energetic electron precipitation (EEP).
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN47635 , COSMIC Data Users'' Workshop; Sep 21, 2017 - Sep 25, 2017; Estes Park, CO; United States|Workshop of the International Radio Occultation Working Group (IROWG); Sep 21, 2017 - Sep 25, 2017; Estes Park, CO; United States
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  • 65
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-40714 , Human Dependability Workshop (HUDEP 2017); Nov 14, 2017 - Nov 16, 2017; Noordwijk; Netherlands
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  • 66
    Publication Date: 2019-07-13
    Description: Background: NASA Strategic Knowledge Gap B5: Forward Contamination for Mars. Issue: we have knowledge gaps!: Whether / how microbes are released from crewed pressure systems. Why do we care?: Informs Mars operational concepts - How to protect the science; Informs architecture decisions - How open Environmental Control and Life Support (ECLS) systems are; Informs landing site selection decisions - How close we can land / operate to where life may be present. Project goal: get some data to fill in these gaps: Data will help determine whether were ready to go to Mars, or if we need to change our systems or operational designs.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-40513 , Extravehicular Activity Technology Workshop 2017; Oct 17, 2017 - Oct 19, 2017; Houston, TX; United States
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  • 67
    Publication Date: 2019-07-13
    Description: Traditional gas-phase trace contaminant control adsorption process flow is constrained as required to maintain high contaminant single-pass adsorption efficiency. Specifically, the bed superficial velocity is controlled to limit the adsorption mass-transfer zone length relative to the physical adsorption bed; this is aided by traditional high-aspect ratio bed design. Through operation in this manner, most contaminants, including those with relatively high potential energy are readily adsorbed. A consequence of this operational approach, however, is a limited available operational flow margin. By considering a paradigm shift in adsorption architecture design and operations, in which flows of high superficial velocity are treated by low-aspect ratio sorbent beds, the range of well-adsorbed contaminants becomes limited, but the process flow is increased such that contaminant leaks or emerging contaminants of interest may be effectively controlled. To this end, the high velocity, low aspect ratio (HVLA) adsorption process architecture was demonstrated against a trace contaminant load representative of the International Space Station atmosphere. Two HVLA concept packaging designs (linear flow and radial flow) were tested. The performance of each design was evaluated and compared against computer simulation. Utilizing the HVLA process, long and sustained control of heavy organic contaminants was demonstrated.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-257 , M17-6319 , International Conference on Environmental Systems (ICES 2017); Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 68
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    In:  CASI
    Publication Date: 2019-07-13
    Description: Presentation on New Space development paradigm.
    Keywords: Space Sciences (General)
    Type: ARC-E-DAA-TN42624 , Asian Space Technology Summit 2017; May 11, 2017; Kuala Lumpur; Malaysia
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  • 69
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-38430 , Human Research Program Investigators'' Workshop; Jan 23, 2017 - Jan 27, 2017; Galveston, TX; United States
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  • 70
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-40501 , Human Factors and Ergonomics Conference; Oct 09, 2017 - Oct 13, 2017; Austin, TX; United States
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  • 71
    Publication Date: 2019-07-13
    Description: The International Planetary Probe Workshop (IPPW) is a forum for exchanging information and encourage collaboration. The IPPW-14 (2017) in its 14th year and attracts participants mainly from US and Europe. The authors of this proposed talk are exploring and have established international collaboration in multiple areas of interest to IPPW community. The authors will present examples that illustrate the motivations for the partnership, the unique capabilities and the potential benefits of international collaboration and how to approach the collaboration in order to overcome the challenges.
    Keywords: Space Sciences (General)
    Type: ARC-E-DAA-TN43025 , International Planetary Probe Workshop; Jun 12, 2017 - Jun 16, 2017; The Hague; Netherlands
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  • 72
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Space Sciences (General)
    Type: M17-6200 , Huntsville Hamfest 2017; Aug 19, 2017 - Aug 20, 2017; Huntsville, AL; United States
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  • 73
    Publication Date: 2019-07-13
    Description: Simulations of six new 4-Bed Molecular Sieve configurations have been performed using a COMSOL model. The preliminary results show that reductions in desiccant bed size and sorbent bed size when compared to the International Space Station configuration are feasible while still yielding a process that handles at least 4.0 kg/day CO2. The results also show that changes to the CO2 sorbent are likewise feasible. Decreasing the bed sizes was found to have very little negative effect on the adsorption process; breakthrough of CO2 in the sorbent bed was observed for two of the configurations, but water breakthrough in the desiccant beds was not observed. Nevertheless, both configurations for which CO2 breakthrough was observed still yield relatively high CO2 efficiency, and future investigations will focus on bed size in order to find the optimum configuration.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-111 , M17-5887 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 74
    Publication Date: 2019-07-13
    Description: Minimizing resupply from Earth is essential for future long duration manned missions. The current oxygen recovery system aboard the International Space Station is capable of recovering approximately 50% of the oxygen from metabolic carbon dioxide. For long duration manned missions, a minimum of 75% oxygen recovery is targeted with a goal of greater than 90%. Theoretically, the Bosch process can recover 100% of oxygen, making it a promising technology for oxygen recovery for long duration missions. However, the Bosch process produces elemental carbon which ultimately fouls the catalyst. Once the catalyst performance is compromised, it must be replaced resulting in undesired resupply mass. Based on the performance of a Bosch system designed by NASA in the 1990's, a three year Martian mission would require approximately 1315 kg (2850 lbs) of catalyst resupply. It may be possible to eliminate catalyst resupply with a fully regenerable system using an Ionic Liquid (IL)-based Bosch system. In 2016, we reported the feasibility of using ILs to produce an iron catalyst on a copper substrate and to regenerate the iron catalyst by extracting the iron from the copper substrate and product carbon. Additionally, we described a basic system concept for an IL-based Bosch. Here we report the results of efforts to scale catalyst preparation, catalyst regeneration, and to scale the carbon formation processing rate of a single reactor.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-308 , M17-5875 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 75
    Publication Date: 2019-07-13
    Description: Human exploration missions to Mars and other destinations beyond low Earth orbit require highly robust, reliable, and maintainable life support systems that maximize recycling of water and oxygen. In order to meet this requirement, NASA has continued the development of a Series-Bosch System, a two stage reactor process that reduces carbon dioxide (CO2) with hydrogen (H2) to produce water and solid carbon. Theoretically, the Bosch process can recover 100% of the oxygen (O2) from CO2 in the form of water, making it an attractive option for long duration missions. The Series Bosch system includes a reverse water gas shift (RWGS) reactor, a carbon formation reactor (CFR), an H2 extraction membrane, and a CO2 extraction membrane. In 2016, the results of integrated testing of the Series Bosch system showed great promise and resulted in design modifications to the CFR to further improve performance. This year, integrated testing was conducted with the modified reactor to evaluate its performance and compare it with the performance of the previous configuration. Additionally, a CFR with the capability to load new catalyst and remove spent catalyst in-situ was built. Flow demonstrations were performed to evaluate both the catalyst loading and removal process and the hardware performance. The results of the integrated testing with the modified CFR as well as the flow demonstrations are discussed in this paper.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-219 , M17-5959 , International Conference on Environmental Systems (ICES) 2017; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 76
    Publication Date: 2019-07-13
    Description: State-of-the-art life support oxygen recovery technology on the International Space Station is based on the Sabatier reaction where only about half of the oxygen required for the crew is recovered from metabolic carbon dioxide (CO2). The Sabatier reaction produces water as the primary product and methane as a byproduct. Oxygen recovery is constrained by both the limited availability of reactant hydrogen from water electrolysis and Sabatier methane (CH4) being vented as a waste product resulting in a continuous loss of reactant hydrogen. Post-processing methane with the Plasma Pyrolysis Assembly (PPA) to recover this hydrogen has the potential to substantially increase oxygen recovery and thus dramatically reduce the logistical challenges associated with oxygen resupply. The PPA decomposes methane into predominantly hydrogen and acetylene. A purification system is necessary to purify hydrogen before it is recycled back to the Sabatier reactor. Testing and evaluation of acetylene removal systems and PPA system architectures are presented and discussed.
    Keywords: Man/System Technology and Life Support
    Type: M17-5961 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 77
    Publication Date: 2019-07-13
    Description: NASA has embarked on an endeavor that will enable humans to explore deep space, with the ultimate goal of sending humans to Mars. This journey will require significant developments in a wide range of technical areas, as resupply is unavailable in the Mars transit phase and early return is not possible. Additionally, mass, power, volume, and other resources must be minimized for all subsystems to reduce propulsion needs. Among the critical areas identified for development are life support systems, which will require increases in reliability and reductions in resources. This paper discusses current and planned developments in the area of carbon dioxide removal to support crewed Mars-class missions.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-209 , M17-6065 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 78
    Publication Date: 2019-07-13
    Description: NASA has embarked on the mission to enable humans to explore deep space, including the goal of sending humans to Mars. This journey will require significant developments in a wide range of technical areas as resupply and early return are not possible. Additionally, mass, power, and volume must be minimized for all phases to maximize propulsion availability. Among the critical areas identified for development are life support systems, which will require increases in reliability as well as reduce resource usage. Two primary points for reliability are the mechanical stability of sorbent pellets and recovery of CO2 sorbent productivity after off-nominal events. In this paper, we discuss the present efforts towards screening and characterizing commercially-available sorbents for extended operation in desiccant and CO2 removal beds. With minimized dusting as the primary criteria, a commercial 13X zeolite was selected and tested for performance and risk.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-188 , M17-6066 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 79
    Publication Date: 2019-07-13
    Description: In support of the NASA goals to reduce power, volume and mass requirements on future CO2 (Carbon Dioxide) removal systems for exploration missions, a 4BMS (Four Bed Molecular Sieve) test bed was fabricated and activated at the NASA Marshall Space Flight Center. The 4BMS-X (Four Bed Molecular Sieve-Exploration) test bed used components similar in size, spacing, and function to those on the flight ISS flight CDRA system, but were assembled in an open framework. This open framework allows for quick integration of changes to components, beds and material systems. The test stand is highly instrumented to provide data necessary to anchor predictive modeling efforts occurring in parallel to testing. System architecture and test data collected on the initial configurations will be presented.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-240 , M17-6072 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 80
    Publication Date: 2019-07-13
    Description: The International Space Station (ISS) program is investigating methods to increase carbon dioxide (CO2) removal on ISS in order to support an increased number of astronauts at a future date. The Carbon Dioxide Removal Assembly - Engineering Unit (CDRA-4EU) system at NASA Marshall Space Flight Center (MSFC) was tested at maximum fan settings to evaluate CO2 removal rate and power consumption at those settings.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-241 , M17-6073 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 81
    Publication Date: 2019-07-13
    Description: The International Space Station (ISS) Water Recovery System (WRS) includes the Water Processor Assembly (WPA) and the Urine Processor Assembly (UPA). The WRS produces potable water from a combination of crew urine (first processed through the UPA), crew latent, and Sabatier product water. Though the WRS has performed well since operations began in November 2008, several modifications have been identified to improve the overall system performance. These modifications aim to reduce resupply and improve overall system reliability, which is beneficial for the ongoing ISS mission as well as for future NASA manned missions. The following paper details efforts to improve the WPA through the use of reverse osmosis membrane technology to reduce the resupply mass of the WPA Multi-filtration Bed and improved catalyst for the WPA Catalytic Reactor to reduce the operational temperature and pressure. For the UPA, this paper discusses progress on various concepts for improving the reliability of the system, including the implementation of a more reliable drive belt, improved methods for managing condensate in the stationary bowl of the Distillation Assembly, and evaluating upgrades to the UPA vacuum pump.
    Keywords: Man/System Technology and Life Support
    Type: ICES-2017-40 , M17-6116 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 82
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Man/System Technology and Life Support
    Type: M17-6149 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 83
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Man/System Technology and Life Support
    Type: M17-6162 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 84
    Publication Date: 2019-07-13
    Description: The US Antarctic Meteorite Program has visited the Dominion Range in the Transantarctic Mountains during several different seasons, including the 1985, 2003, 2008, 2010, and 2014 seasons. Total recovered meteorites from this region is over 2000. The 1985 (11 samples), 2003 (141 samples), 2008 (521) and 2010 (901 samples) seasons have been fully classified, and the 2014 samples (562) are in the process of being classified and characterized. Given that close to 1500 samples have been classified so far, it seems like a good opportunity to summarize the state of the collection. Here we describe the significant samples documented from this area, as well as a large meteorite shower that dominates the statistics of the region.
    Keywords: Space Sciences (General)
    Type: JSC-CN-40505 , 2017 Hayabusa Symposium of the Solar System Materials; Dec 04, 2017 - Dec 07, 2017; Tokyo; Japan
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  • 85
    Publication Date: 2019-07-13
    Description: We describe an Evolved Expendable Launch Vehicle Secondary Payload Adapter (ESPA)-class SmallSat spinning lander concept for the exploration of Europa or other Ocean World surfaces to ascertain the potential for life. The spinning lander will be ejected from an ESPA ring from an orbiting or flyby spacecraft and will carry on-board a standoff remote Spatial Heterodyne Raman spectrometer (SHRS) and a time resolved laser induced fluorescence spectrograph (TR-LIFS), and once landed and stationary the instruments will make surface chemical measurements. The SHRS and TR-LIFS have no moving parts have minimal mass and power requirements and will be able to characterize the surface and near-surface chemistry, including complex organic chemistry to constrain the ocean composition.
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN42646 , European Planetary Science Congress 2017 Meeting; Sep 17, 2017 - Sep 22, 2017; Riga; Latvia
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  • 86
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Space Sciences (General)
    Type: MSFC-E-DAA-TN40056 , COSPAR Small Satellite Symposium; Sep 18, 2017 - Sep 22, 2017; Jeju; Korea, Republic of
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  • 87
    facet.materialart.
    Unknown
    In:  CASI
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-40432 , Industrial Fabric Association International (IFAI) Expo 2017; Sep 26, 2017 - Sep 29, 2017; New Orleans, LA; United States
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  • 88
    Publication Date: 2019-07-13
    Description: A recent improvement to the long-term estimation of ground casualties from reentering space debris is the further refinement and update to the human population distribution. Previous human population distributions were based on global totals with simple scaling factors for future years, or a coarse grid of population counts in a subset of the world's countries, each cell having its own projected growth rate. The newest population model includes a 5-fold refinement in both latitude and longitude resolution. All areas along a single latitude are combined to form a global population distribution as a function of latitude, creating a more accurate population estimation based on non-uniform growth at the country and area levels. Previous risk probability calculations used simplifying assumptions that did not account for the ellipsoidal nature of the Earth. The new method uses first, a simple analytical method to estimate the amount of time spent above each latitude band for a debris object with a given orbit inclination and second, a more complex numerical method that incorporates the effects of a non-spherical Earth. These new results are compared with the prior models to assess the magnitude of the effects on reentry casualty risk.
    Keywords: Space Sciences (General)
    Type: JSC-CN-40468 , International Association for the Advancement of Space Safety (IAASS) Conference; Oct 18, 2017 - Oct 20, 2017; Toulouse; France
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  • 89
    Publication Date: 2019-07-13
    Description: Microwave-based plasma pyrolysis technology is being studied as a means of supporting oxygen recovery in future spacecraft life support systems. The process involves the conversion of methane produced from a Sabatier reactor to acetylene and hydrogen, with a small amount of solid carbon particulates generated as a side product. The particles must be filtered before the acetylene is removed and the hydrogen-rich gas stream is recycled back to the CRA. We discuss developmental work on porous metal media filters for removing the carbon particulate emissions from the PPA exit gas stream and to provide in situ media regeneration capability. Because of the high temperatures involved in oxidizing the deposited carbon during regeneration, there was particular focus in this development on the materials that could be used, the housing design, and heating methods. This paper describes the design and operation of the filter and characterizes their performance from integrated testing at the Environmental Chamber (E-Chamber) at MSFC.
    Keywords: Man/System Technology and Life Support
    Type: GRC-E-DAA-TN44367 , International Conference on Environmental Systems; Jul 16, 2017 - Jul 20, 2017; Charleston, SC; United States
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  • 90
    Publication Date: 2019-07-13
    Description: Mid- and far-infrared spectra of condensed ethanol (CH3CH2OH) at 10-160 K are presented, with a special focus on amorphous ethanol, the form of greatest astrochemical interest, and with special attention given to changes at 155-160 K. Infrared spectra of amorphous and crystalline forms are shown. The refractive index at 670 nm of amorphous ethanol at 16 K is reported, along with three IR band strengths and a density. A comparison is made to recent work on the isoelectronic compound ethanethiol (CH3CH2SH), and several astrochemical applications are suggested for future study.
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN45485 , Spectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy (ISSN 1386-1425); 187; 82-86
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  • 91
    Publication Date: 2019-07-13
    Description: The NASA Orbital Debris Program Office (ODPO) recently commissioned the Meter Class Autonomous Telescope (MCAT) on Ascension Island with the primary goal of obtaining population statistics of the geosynchronous (GEO) orbital debris environment. To help facilitate this, studies have been conducted using MCAT's known and projected capabilities to estimate the accuracy and timeliness in which it can survey the GEO environment. A simulated GEO debris population is created and sampled at various cadences and run through the Constrained Admissible Region Multi Hypotheses Filter (CAR-MHF). The orbits computed from the results are then compared to the simulated data to assess MCAT's ability to determine accurately the orbits of debris at various sample rates. Additionally, estimates of the rate at which MCAT will be able produce a complete GEO survey are presented using collected weather data and the proposed observation data collection cadence. The specific methods and results are presented here.
    Keywords: Space Sciences (General)
    Type: JSC-CN-40380 , Advanced Maui Optical and Space Surveillance Conference; Sep 19, 2017 - Sep 22, 2017; Maui, HI; United States
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  • 92
    Publication Date: 2019-07-13
    Description: The National Aeronautics and Space Administration (NASA) has led in the development of unique flame retardant fibers for human spaceflight since the beginning of the Apollo program. After the Apollo 1 fire which killed Command Pilot Virgil I 'Gus' Grissom, Senior Pilot Edward H. White II, and Pilot Roger B. Chaffee from cardiac arrest on January 27, 1967, the accident investigators found severe third degree burns and melted spacesuits on the astronauts bodies. NASA immediately initiated an extensive research program aimed at developing flame retardant and flame resistant fibers for the enriched oxygen atmosphere of the Apollo crew cabin. Fibers are flame retardant when they have been modified by chemical and thermal treatments. Fibers are flame resistant when they are made of inherently flame resistant materials (i.e. glass, ceramic, highly aromatic polymers). Immediately after this tragic accident, NASA funded extensive research in specifically developing flame retardant fibers and fabrics. The early developmental efforts for human spaceflight were for the outer layer of the Apollo spacesuit. It was imperative that non-flammable fabrics be used in a 100% oxygen environment. Owens-Corning thus developed the Beta fiber that was immediately used in the Apollo program and later in the Space Shuttle program. Aside from the urgent need for protective fabrics for the spacesuit, NASA also needed flame retardant fabrics for both clothing and equipment inside the spacecraft. From the mid-1960s to the early 1980's, NASA contracted with many companies to develop inherently flame retardant fibers and flame retardant finishes for existing fibers. Fluorocarbons and aromatic polyamides were the polymers of great interest for the development of new inherently flame retardant fibers for enriched oxygen environments. These enriched environments varied for different space programs. For example, the Apollo program requirements were for materials that would not support combustion in a 70%/30% oxygen/nitrogen environment at 6.3 pounds per square inch (psi). The Skylab program flammability requirements were set at 80%/20% oxygen/nitrogen ratios at 5 psi. While many fibers produced under several NASA contracts were never used, a few have become commercial products. The intent of this paper is to present the developmental history of some of these new or modified textile fibers. These developmental efforts are presented at various levels of details depending on the source of the historical records.
    Keywords: Man/System Technology and Life Support
    Type: JSC-CN-40369 , Dornbirn Man-Made Fibers Congress; Sep 13, 2017 - Sep 15, 2017; Dornbirn; Austria
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  • 93
    Publication Date: 2019-07-13
    Description: We re-examine the radio and plasma wave observations obtained during the Cassini Saturn orbit insertion period, as the spacecraft flew over the northern ring surface into a radial distance of 1.3 Rs (over the C-ring). Voyager era studies suggest the rings are a source of micro-meteoroid generated plasma and dust, with theorized peak impact-created plasma outflows over the densest portion of the rings (central B-ring). In sharp contrast, the Cassini Radio and Plasma Wave System (RPWS) observations identify the presence of a ring-plasma cavity located in the central portion of the B-ring, with little evidence of impact-related plasma. While previous Voyager era studies have predicted unstable ion orbits over the C- ring, leading to field-aligned plasma transport to Saturns ionosphere, the Cassini RPWS observations do not reveal evidence for such instability-created plasma fountains. Given the passive ring loss processes observed by Cassini, we find that the ring lifetimes should extend 〉10(exp 9) years, and that there is limited evidence for prompt destruction (loss in 〈100 Myrs).
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN45495 , Icarus (ISSN 0019-1035); 292; 48-53
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  • 94
    Publication Date: 2019-07-13
    Description: A first complete draft of the Simulation Interoperability Standards Organization (SISO) Space Reference Federation Object Model (FOM) has now been produced. This paper provides some insights into its capabilities and discusses the opportunity for reuse in other domains. The focus of this first version of the standard is execution control, time management and coordinate systems, well-known reference frames, as well as some basic support for physical entities. The biggest part of the execution control is the coordinated start-up process. This process contains a number of steps, including checking of required federates, handling of early versus late joiners, sharing of federation wide configuration data and multi-phase initialization. An additional part of Execution Control is the coordinated and synchronized transition between Run mode, Freeze mode and Shutdown. For time management, several time lines are defined, including real-time, scenario time, High Level Architecture (HLA) logical time and physical time. A strategy for mixing simulations that use different time steps is introduced, as well as an approach for finding common boundaries for fully synchronized freeze. For describing spatial information, a mechanism with a set of reference frames is specified. Each reference frame has a position and orientation related to a parent reference frame. This makes it possible for federates to perform calculations in reference frames that are convenient to them. An operation on the Moon can be performed using lunar coordinates whereas an operation on Earth can be performed using Earth coordinates. At the same time, coordinates in one reference frame have an unambiguous relationship to a coordinate in another reference frame. While the Space Reference FOM is originally being developed for Space operations, the authors believe that many parts of it can be reused for any simulation that has a focus on physical processes with one or more coordinate systems, and require high fidelity and repeatability.
    Keywords: Space Sciences (General)
    Type: JSC-CN-40073 , Simulation Innovation Workshop (SIW) Simulation Interoperability Standards Organization (SISO); Sep 10, 2017 - Sep 15, 2017; Orlando, FL; United States
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  • 95
    Publication Date: 2019-07-13
    Description: The Vegetable Production System (Veggie) is a scientific payload designed to support plant growth for food production under microgravity conditions. The configuration of Veggie consists of an LED lighting system with modular rooting pillows designed to contain substrate media and time-release fertilizer. The pillows were designed to be watered passively using capillary principles but have typically been watered manually by the astronauts in low-Earth orbit (LEO). The design of Veggie allows cabin air to be drawn through the plant enclosure for thermal and humidity control and for supplying CO2 to the plants. Since its delivery to the International Space Station (ISS) in 2014, Veggie has undergone several experimental trials by various crews. Ground unit testing of Veggie was conducted during an 8-month Mars analog study in a semi-contained environment of a simulated habitat located at approximately 8,200 feet (2,500 m) elevation on the Mauna Loa volcano on the Island of Hawaii. The Hawaii Space Exploration Analog and Simulation (HI-SEAS) offered conditions (habitat, mission, communications, etc.) intended to simulate a planetary exploration mission. This paper provides data and analyses to show the prospect for optimized use of the current Veggie design for human habitats. Lessons learned during the study may provide opportunities for updating the system design and operational parameters for current Veggie experiments being conducted onboard the ISS and for payloads on future deep space missions.
    Keywords: Man/System Technology and Life Support
    Type: KSC-E-DAA-TN45420 , AIAA SPACE Forum 2017; Sep 12, 2017 - Sep 14, 2017; Orlando, FL; United States
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  • 96
    Publication Date: 2019-07-13
    Description: Over a million individually measured meteoroid orbits were collected with the Southern Argentina Agile MEteor Radar (SAAMER) between 2012-2015. This provides a robust statistical database to perform an initial orbital survey of meteor showers in the Southern Hemisphere via the application of a 3D wavelet transform. The method results in a composite year from all 4 years of data, enabling us to obtain an undisturbed year of meteor activity with more than one thousand meteors per day. Our automated meteor shower search methodology identified 58 showers. Of these showers, 24 were associated with previously reported showers from the IAU catalogue while 34 showers are new and not listed in the catalogue. Our searching method combined with our large data sample provides unprecedented accuracy in measuring meteor shower activity and description of shower characteristics in the Southern Hemisphere. Using simple modeling and clustering methods we also propose potential parent bodies for the newly discovered showers.
    Keywords: Space Sciences (General)
    Type: GSFC-E-DAA-TN45798 , ICARUS (ISSN 0019-1035) (e-ISSN 1090-2643); 290; 162–182
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  • 97
    Publication Date: 2019-07-19
    Description: Controlled Environment Agriculture (CEA) systems can be used to produce high-quality, desirable food year round, and the fresh produce can positively contribute to the health and well being of residents in communities with difficult supply logistics. While CEA has many positive outcomes for a remote community, the associated high electric demands have prohibited widespread implementation in what is typically already a fully subscribed power generation and distribution system. Recent advances in CEA technologies as well as renewable power generation, storage, and micro-grid management are increasing system efficiency and expanding the possibilities for enhancing community supporting infrastructure without increasing demands for outside supplied fuels. We will present examples of how new lighting, nutrient delivery, and energy management and control systems can enable significant increases in food production efficiency while maintaining high yields in CEA.Examples from Alaskan communities where initial incorporation of renewable power generation, energy storage and grid management techniques have already reduced diesel fuel consumption for electric generation by more than 40 and expanded grid capacity will be presented. We will discuss how renewable power generation, efficient grid management to extract maximum community service per kW, and novel energy storage approaches can expand the food production, water supply, waste treatment, sanitation and other community support services without traditional increases of consumable fuels supplied from outside the community. These capabilities offer communities with a range of choices to enhance their communities. The examples represent a synergy of technology advancement efforts to develop sustainable community support systems for future space-based human habitats and practical implementation of infrastructure components to increase efficiency and enhance health and well-being in remote communities today and tomorrow.
    Keywords: Man/System Technology and Life Support
    Type: ARC-E-DAA-TN46611 , Lecture at the at Norwegian Institute of Bioeconomy; Oct 12, 2017 - Oct 20, 2017; Tromso; Norway
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  • 98
    facet.materialart.
    Unknown
    In:  CASI
    Publication Date: 2019-07-19
    Description: Burns et al. (1979) use the parameter beta to describe the ratio of radiation pressure to gravity for a particle in the Solar System. The central potential that these particles experience is effectively reduced by a factor of (1- beta ), which in turn lowers the escape velocity. Burns et al. (1979) derived a simple expression for the value of beta at which particles ejected from a comet follow parabolic orbits and thus leave the Solar System; we expand on this to derive an expression for critical beta values that takes ejection velocity into account, assuming geometric optics. We use our expression to compute the critical value and corresponding mass for cometary ejecta leading, trailing, and following the parent comet's nucleus for 10 major meteor showers. Finally, we numerically solve for critical beta values in the case of non-geometric optics. These values determine the mass regimes within which meteoroids are ejected from the Solar System and therefore cannot contribute to meteor showers.
    Keywords: Space Sciences (General)
    Type: M17-6070 , Division for Planetary Sciences (DPS) 2017 Annual Meeting; Oct 15, 2017 - Oct 20, 2017; Provo, UT; United States
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  • 99
    Publication Date: 2019-07-19
    Description: The ISS WRS produces potable water from crew urine, crew latent, and Sabatier product water. This system has been operational on ISS since November 2008, producing over 30,000 L of water during that time. The WRS includes a Urine Processor Assembly (UPA) to produce a distillate from the crew urine. This distillate is combined with the crew latent and Sabatier product water and further processed by the Water Processor Assembly (WPA) to the potable water. The UPA and WPA use technologies commonly used on ISS for water purification, including filtration, distillation, adsorption, ion exchange, and catalytic oxidation. The primary challenge with the design and operation of the WRS has been with implementing these technologies in microgravity. The absence of gravity has created unique issues that impact the constituency of the waste streams, alter two-phase fluid dynamics, and increases the impact of particulates on system performance. NASA personnel continue to pursue upgrades to the existing design to improve reliability while also addressing their viability for missions beyond ISS.
    Keywords: Man/System Technology and Life Support
    Type: M17-6277 , Annual Meeting of the American Society for Gravitational and Space Research (ASGSR 2017); Oct 25, 2017 - Oct 28, 2017; Renton, WA; United States
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  • 100
    Publication Date: 2019-07-19
    Description: Throughout the human space flight program there have been instances where smoke, fire, and pressure loss have occurred onboard space vehicles, putting crews at risk for loss of mission and loss of life. In every instance the mission has been in Low-Earth-Orbit (LEO) with access to multiple volumes that could be used to quickly seal off the damaged module or escape vehicles for a quick return to Earth. For long duration space missions beyond LEO, including Mars transit missions of about 1000 days, the mass penalty for multiple volumes has been a concern as has operating in an environment where a quick return will not be possible. In 2016 a study was done to investigate a variety of dual pressure vessel configurations for habitats that could protect the crew from these hazards. It was found that for a modest increase in total mass it should be possible to provide significant protection for the crew. Several configurations were developed that either had a small safe haven to provide 30-days to recover, or a full duration safe haven using two equal size pressure vessel volumes. The 30-day safe haven was found to be the simplest, yielding the least total mass impact but still with some risk if recovery is not possible during that timeframe. The full duration safe haven was the most massive option but provided the most robust solution. This paper provides information on the various layouts considered in the study and provides a discussion of the findings for implementing a safe haven in future habitat designs.
    Keywords: Man/System Technology and Life Support
    Type: M17-5955 , AIAA Space and Astronautics Forum and Exposition; Sep 12, 2017 - Sep 14, 2017; Orlando, FL; United States
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