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  • LUNAR AND PLANETARY EXPLORATION  (111)
  • Inorganic Chemistry  (43)
  • 1985-1989  (154)
  • 1980-1984
  • 1970-1974
  • 1950-1954
  • 1987  (154)
Collection
Publisher
Years
  • 1985-1989  (154)
  • 1980-1984
  • 1970-1974
  • 1950-1954
Year
  • 1
    Publication Date: 2019-07-12
    Description: Observations of electrostatic waves in the magnetosphere of Uranus are discussed with attention focused on the Bernstein emissions. The most intense Bernstein waves were observed near the magnetic equator of the planet, even though the tilt of the Uranian magnetic moment is very large relative to the rotational axis. In addition to the Bernstein modes, a number of highly sporadic emissions were detected in the vicinity of the Miranda L shell.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Journal of Geophysical Research (ISSN 0148-0227); 92; 15225-15
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  • 2
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: The Thermal Behaviour of Caesiumchloroferrates(III) and Caesiumehloroferrate(III) Hydrates. II. The Rehydration of Decomposition Products of Cs3[FeCl6]  -  A Raman Spectroscopic Study under Definite Atmosphere of Water VapourCs3[FeCl6] formed by dehydration of Cs3[FeCl6] · H2O at about 160°C does not change at normal atmosphere within 3 till 4 hours. Rehydration under the vapour pressure of the eliminated water yields the monohydrate in nearly the same time. In the same manner rehydration of the solid mixture of Cs[FeCl4] and 2 CsCl formed by thermal decomposition of the metastable Cs3[FeCl6] (280°C) produces the intermediates Cs3[Fe2Cl9] and Cs2[Fe(H2O)Cl5] in mixtures with CsCl and, finally, Cs3[FeCl6] · H2O. The formation of Cs3[Fe2Cl9] from Cs[FeCl4] and CsCl is accelerated by water. The reaction cycle has been studied using Raman and IR spectroscopy. The results will be discussed with respect to thermoanalytical data.
    Notes: Wasserfreies Cs3[FeCl6], das durch Entwässerung des Monohydrates bei etwa 160°C gebildet wird, zeigt an der Raumluft innerhalb von 3 bis 4 Stunden keine Veränderungen. Dagegen erfolgt unter dem Dampfdruck des abgespaltenen Wassers in etwa der gleichen Zeit die Rehydratation zu Cs3[FeCl6] · H2O. Auch die Rehydratation des bei der thermischen Zersetzung von metastabilem Cs3[FeCl6] (280°C) gebildeten festen Gemisches von Cs[FeCl4] und 2 CsCl führt über die Zwischenstufen Cs3[Fe2Cl9] und Cs2[Fe(H2O)Cl5] im Gemisch mit CsCl wieder zum Cs3[FeCl6] · H2O. Das Wasser wirkt bei der Bildung von Cs3[Fe2Cl9] aus Cs[FeCl4] und CsCl reaktionsbeschleunigend.Der Reaktionszyklus wird mittels Raman- und IR-Spektroskopie untersucht. Die Ergebnisse werden mit simultanthermoanalytischen Befunden verglichen.
    Additional Material: 3 Ill.
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  • 3
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Zeitschrift für anorganische Chemie 544 (1987), S. 159-166 
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: Fluoride und Fluorosäuren. XI. Polyhydrogenfluoride mit dem Tetramethylammonium-Kation: Darstellung, Stabilitätsbereiche, Kristallstrukturen, [HnFn+1]--Anion-Homologie, Wasserstoffbrücken F—H…FDas Schmelzdiagramm des Systems (CH3)4NF—HF wurde zwischen 50 und 100 Mol-% HF und von -185°C bis zu den jeweiligen Liquidustemperaturen (maximal 162°C) mit Differenzthermoanalyse, unterstützt durch temperaturabhängige Röntgen-Pulverbeugung, untersucht. Das System wurde als quasibinär erkannt mit den HF-reichen intermediären stabilen Verbindungen (CH3)4NF · 2 HF (Schmelzpunkt 110°C), (CH3)4NF · 3 HF (20°C, Zersetzung), (CH3)4NF · 5 HF (-76°C, Zersetzung) und (CH3)4NF · 7 HF (-110°C, Zersetzung), von denen die meisten Phasenumwandlungen fest-fest durchlaufen. Kristallstrukturen wurden bestimmt von der Tieftemperaturform von (CH3)4NF · 2 HF (stabil unterhalb von 83°C, orthorhombisch, Raumgruppe Pbca, Z = 8 Formeleinheiten pro Elementarzelle), der Hochtemperaturform von (CH3)4NF · 3 HF (stabil oberhalb von -87°C, monokolin, P2/c, Z = 4) und von (CH3)4NF · 5 HF (tetragonal, 14, Z = 2). Die Strukturen sind solche von Polyhydrogenfluoriden (CH3)4N[HnFn+1] mit homologen Anionen [H2F3]- bzw. [H3F4]- und [H5F6-], die durch starke Wasserstoffbrücken F—H…F gebildet werden. Das Anion [H5F6,]- ist das erste dieser Zusammensetzung, das durch Kristallstrukturbestimmung etabliert wurde. Seine Struktur kann als [(FH)2FHF(HF)2]- geschrieben werden mit vier äquivalenten terminalen Wasserstoffbrücken von 248.4 pm und einer sehr kurzen zentralen von 226.6 pm (F…F- Abstände) durch einen Punkt der Ranmgruppe.
    Notes: The melting diagram of the system (CH3)4NF—HF was studied between 50 and 100 mole-% HF and from -185°C to the respective liquidus temperatures (at most 162°C) by difference thermal analysis aided by temperature-dependent X-ray powder diffraction. The system was found to be quasi-binary with the HF-rich intermediary stable compounds (CH3)4NF · 2 HF (melting point 110°C), (CH3)4NF · 3 HF (20°C, decomposition), (CH3)4NF · 5 HF (-76°C, decomposition), and (CH3)4NF · 7 HF (-110°C, decomposition), most of which undergo solid-solid phase transitions. Crystal structures were determined of the low-temperature form of (CH3)4NF · 2 HF (stable below 83°C, orthorhombic, space group Pbca, Z = 8 formula units per unit cell), the high-temperature form of (CH3)4NF · 3 HF (stable above -87°C, monoclinic, P2/c, Z = 4), and of (CH3)4NF · 5 HF (tetragonal, I4, Z = 2). The structures are those of poly(hydrogen fluorides) (CH3)4N[HnFn+1] with homologous anions [H2F3]-, [H3F4]-, and [H5F6]-, respectively, formed by strong hydrogen bonding F—H…F. The anion [H5F6]- is the first one of this composition established by crystal structure analysis. Its structure can be written as [(FH)2FHF(HF)2]- with four equivalent terminal hydrogen bonds of 248.4 pm and a very short central one of 226.6 pm (F…F distances) through a 4 point of the space group.
    Additional Material: 3 Ill.
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  • 4
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: Contributions to the Chemistry of Phosphorus. 172. Existence and Characterization of the Pentaphosphacyclopentadienide Anion, P5-, the Tetraphosphacyclopentadienide Ion, P4CH-, and the Triphosphacyclobutenide Ion, P3CH2-The pentaphosphacyclopentadienide anion, P5- (1), the tetraphosphacyclopentadienide ion, P4CH-(2), and the triphosphacyclobutenide ion, P3CH2-(3), are formed besides other polyphosphides by the nucleophilic cleavage of white phosphorus with sodium in diglyme. 1 also results from the reaction of lithium dihydrogenphosphide with white phosphorus and can be obtained pure in the form of a LiP5 solution after separating the other products. The common structural feature of 1, 2, and 3 are rings with unsubstituted P atoms of coordination number 2 that are stabilized by mesomerism.
    Notes: Das Pentaphosphacyclopentadienid-Anion, P5-(1), das Tetraphosphacyclopentadienid-Ion, P4CH- (2), und das Triphosphacyclobutenid-Ion, P3CH2- (3), werden bei der nucleophilen Spaltung von weißem Phosphor mit Natrium in Diglyme neben weiteren Polyphosphiden gebildet. 1 entsteht auch bei der Reaktion von Lithiumdihydrogenphosphid mit weißem Phosphor und kann nach Abtrennung der anderen Produkte in Form einer LiP5-Lösung rein erhalten werden. 1, 2 und 3 weisen als gemeinsames Strukturmerkmal mesomeriestabilisierte Ringe mit unsubstituierten P-Atomen der Koordinationszahl 2 auf.
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  • 5
    Publication Date: 2011-08-19
    Description: The Uranian atmosphere is investigated on the basis of S-band and X-band occultation observations (including measurements of Doppler frequency perturbations) obtained during the Voyager 2 encounter with Uranus in January 1986. The data are presented in extensive tables and graphs and characterized in detail. The atmosphere is assumed to have an H2/He abundance ratio of about 85/15, but also to contain small amounts of CH4 at above-cloud relative humidity 30 percent, cloud-base relative humidity 78 percent, and below-cloud mixing ratio 2.3 percent by number density. Other parameters estimated include magnetic-field rotation period 17.24 h, 1-bar equatorial radius 25,559 + or - 4 km, polar radius 24,973 + or - 20 km, equatorial acceleration of gravity 8.69 + or - 0.01 m/sec sq, and atmospheric temperature 76 + or - 2 K (assuming 85 + or - 3 percent H2).
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Journal of Geophysical Research (ISSN 0148-0227); 92; 14987-15
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  • 6
    Publication Date: 2011-08-19
    Description: Two aluminous mare basalt clasts of high K abundances from Apollo 14 breccia 14304 (the 14304,127 and 14304,128 samples) were characterized with respect to the Rb and Sr concentrations and isotopic compositions, and the Rb-Sr, K-Ar, and Sm-Nd isotopic age determinations were carried out. The results suggest that these high-K basalts were melts derived from mantle material and that they have experienced about ten-fold Rb/Sr and K/La enrichments at approximately the time of crystallization.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Geochimica et Cosmochimica Acta (ISSN 0016-7037); 51; 3255-327
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  • 7
    Publication Date: 2019-06-28
    Description: In order to derive models of the interiors of Uranus, Neptune, Jupiter and Saturn, researchers studied equations of state and electrical conductivities of molecules at high dynamic pressures and temperatures. Results are given for shock temperature measurements of N2 and CH4. Temperature data allowed demonstration of shock induced cooling in the the transition region and the existence of crossing isotherms in P-V space.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986; p 141-143
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  • 8
    Publication Date: 2019-06-28
    Description: The RPA2-Positive Ion Cluster Composition Analyzer (PICCA) on the Giotto spacecraft detected 5 mass peaks with regular spacing of 15 amu up to approximately 120 amu. Starting at 45 amu, the peaks decrease in intensity with increasing mass. Within their half-width they are in good agreement with dissociation products of formaldehyde polymer (POM). A production sequence in which cosmic radiation formed POM from water and carbon monoxide on grains that were aggregated into cometesimals is suggested. Other polymers, possibly containing CN, may also exist. Observations suggest that at least some of the H-, C-, and O-containing dust particles detected by the Particle Impact Analyzer (PIA) on board the Giotto spacecraft and its equivalent on the VEGA-1 and -2 spacecraft contain POM. The properties of POM are consistent with many of the unexpected observations in the coma.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: ESA, Proceedings of the International Symposium on the Diversity and Similarity of Comets; p 163-167
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  • 9
    Publication Date: 2019-08-14
    Description: A wide variety of experiments can be conducted on the Space Station that involve the physics of small particles of planetary significance. Processes of interest include nucleation and condensation of particles from a gas, aggregation of small particles into larger ones, and low velocity collisions of particles. All of these processes could be investigated with a general purpose facility on the Space Station. The microgravity environment would be necessary to perform many experiments, as they generally require that particles be suspended for periods substantially longer than are practical at 1 g. Only experiments relevant to planetary processes will be discussed in detail here, but it is important to stress that a particle facility will be useful to a wide variety of scientific disciplines, and can be used to address many scientific problems.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA, Lyndon B. Johnson Space Center, Experiments in Planetary and Related Sciences and the Space Station; 4 p
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  • 10
    Publication Date: 2019-07-12
    Description: Phase-coherent Doppler data generated by the Deep Space Network with the radio communication system during the Voyager 2 encounter with Uranus in January 1986, optical navigation data generated by the Voyager Navigation Team with the Voyager 2 imaging system, and ground-based astrometric data obtained over an 8-yr period are compiled and analyzed to determine the masses and densities of Uranus and its principal satellites. The data-analysis procedures are explained in detail, and the results are presented in tables and graphs. The mean density of Uranus is found to be 1.285 + or - 0.001 g/cu cm, whereas the mean uncompressed mass of all five satellites is 1.48 + or - 0.06 g/cu cm, or 0.10 g/cu cm above the density expected for a homogeneous solar mix of rock, H2O and NH3 ice, and CH4 as clathrate hydrate. This difference is tentatively attributed to the presence of 15 mass percent of pure graphite, which would provide the thermal conductivity required to keep the satellites cold and undifferentiated.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Journal of Geophysical Research (ISSN 0148-0227); 92; 14877-14
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