ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
  • 1
    Publication Date: 2018-06-06
    Description: Since 2008 the VLBI group at the Institute of Geodesy and Geophysics at TU Vienna has focused on the development of a new VLBI data analysis software called VieVS (Vienna VLBI Software). One part of the program, currently under development, is a unit for parameter estimation in so-called global solutions, where the connection of the single sessions is done by stacking at the normal equation level. We can determine time independent geodynamical parameters such as Love and Shida numbers of the solid Earth tides. Apart from the estimation of the constant nominal values of Love and Shida numbers for the second degree of the tidal potential, it is possible to determine frequency dependent values in the diurnal band together with the resonance frequency of Free Core Nutation. In this paper we show first results obtained from the 24-hour IVS R1 and R4 sessions.
    Keywords: Geophysics
    Type: Proceedings of the Sixth General Meeting of the International VLBI Service for Geodesy and Astrometry; 202-206; NASA/CP-2010-215864
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 2
    Publication Date: 2019-06-28
    Description: The line fluxes of the C IV 1550 A and semiforbidden C III 1909 A emission lines in HH 1 are noted to have monotonically decreased by factors of 4-6 between 1979 and 1983, despite a lack of indications of optical range changes. The thickness of the shocked layers and preshock density can be estimated on the basis of these rapid changes, with results suggesting a clumpy medium that leads to truncated shock waves with column densities insufficient for the development of complete recombination zones.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X); 292; L75-L78
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 3
    Publication Date: 2019-06-28
    Description: Short- and long-wavelength IUE spectra of the rather strongly reddened, high radial velocity Herbig-Haro object HH 32A have been obtained. The object is well known for its large positive radial velocity and for its unusually large velocity dispersion. In consequence of the large ultraviolet extinction, the spectra are faint. The semiforbidden C III 1909 and Mg II 2800 emission lines are, however, clearly detected, and their fluxes can be measured with reasonable accuracy. C IV 1550 and Si III 1892 are very probably present. The continuum can be detected convincingly in the wavelength range 1500-1900 A. In other regions it is just barely detectable. The continuum has an energy distribution which is probably very similar to that of HH 1 and HH 2H. If an average galactic extinction curve is used, the line fluxes for semiforbidden C III 1909 and C IV 1550 indicate a shock velocity of at least 140 km/s which is higher than for HH 1 or HH 2. If a Theta Ori-type extinction curve is used instead, ultraviolet line ratios are obtained which are rather similar to those in HH 1 and HH 2.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 277; 216-219
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 4
    Publication Date: 2019-06-28
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 263
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 5
    Publication Date: 2021-03-29
    Description: Die südlichen Anden sind Teil des aktiven Kontinentalrandes von Südamerika, der durch eine Kombination subduktionsgebundener Prozesse gebildet wurde. Die andine Gebirgskette erstreckt sich über den gesamten südamerikanischen Kontinent, variiert jedoch merklich in Höhe und Krustenmächtigkeit. Während die Zentralen Anden, vor allem auch die tieferen Strukturen bis in den oberen Mantel, vergleichsweise gut erforscht sind (SFB267), ist über den geophysikalischen Aufbau der südlichen Anden bisher relativ wenig bekannt. Aus diesem Grund wurde das seismische Experiment ISSA2000 in den südlichen Anden durchgeführt. In dieser Arbeit wurde mithilfe der Methode der lokalen Erdbebentomographie ein 3-D Modell der seismischen Geschwindigkeitstruktur erstellt. Die gleichzeitig durchgeführte Lokalisierung der registrierten Erdbeben, ergibt darüberhinaus ein detailliertes Bild der Verteilung der Seismizität im Untersuchungsgebiet. Im Rahmen des ISSA2000-Experimentes wurde ein seismologisches Netzwerk mit 62 Seismographen betrieben, das die Subduktionszone von der Küste bis in den backarc zwischen 36ʿ und 40ʿS überdeckt. Die Hypozentren der 440 lokalen Erdbeben zeigen eine ~30ʿ geneigte Wadati-Benioff-Zone mit kontinuierlicher Seismizität bis in 120km Tiefe, die vereinzelt bis in 200km Tiefe zu beobachten ist. Sowohl die generell geringe Seismizität im Untersuchungsgebiet als auch die geringe Tiefenerstreckung der Wadati-Benioff-Zone u.a. im Vergleich zu den Zentralen Anden sowie die Konzentration der mitteltiefen Erdbeben in 60km Tiefe, spiegeln wahrscheinlich den Einfluß des jungen Alters und des damit verbundenen hohen thermischen Zustandes der Nazca-Platte auf das Subduktionsregime wider. Das tomographische Vp Modell zeigt zum ersten Mal die Geschwindigkeitsstruktur der südlichen Anden bis in eine Tiefe von 100km. Die Nazca-Platte ist durch die Lage der Erdbeben definiert und durch hohe Vp Geschwindigkeiten gekennzeichnet (7,2-8,3km/s). Die durchschnittlichen Geschwindigkeiten in der kontinentalen Kruste sind im gesamten Vp Modell relativ hoch (5,5-6,5km/s) ...
    Description: thesis
    Keywords: 551
    Language: German
    Type: monograph , publishedVersion
    Format: 137 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 6
    Publication Date: 2002
    Keywords: Seismicity ; Deep seismic sounding (espec. cont. crust) ; Velocity ; Lueth ; Luth
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 7
    Publication Date: 2011-08-24
    Description: Microbialites are organosedimentary structures that can be constructed by a variety of metabolically distinct taxa. Consequently, microbialite structures abound in the fossil record, although the exact nature of the biogeochemical processes that produced them is often unknown. One such class of ancient calcareous structures, Epiphyton and Girvanella, appear in great abundance during the Early Cambrian. Together with Archeocyathids, stromatolites and thrombolites, they formed major Cambrian reef belts. To a large extent, Middle to Late Cambrian reefs are similar to Precambrian reefs, with the exception that the latter, including terminal Proterozoic reefs, do not contain Epiphyton or Girvanella. Here we report the discovery in Pavilion Lake, British Columbia, Canada, of a distinctive assemblage of freshwater calcite microbialites, some of which display microstructures similar to the fabrics displayed by Epiphyton and Girvanella. The morphologies of the modern microbialites vary with depth, and dendritic microstructures of the deep water (〉 30 m) mounds indicate that they may be modern analogues for the ancient calcareous structures. These microbialites thus provide an opportunity to study the biogeochemical interactions that produce fabrics similar to those of some enigmatic Early Cambrian reef structures.
    Keywords: Geosciences (General)
    Type: Nature (ISSN 0028-0836); Volume 407; 6804; 626-9
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 8
    Publication Date: 2011-08-19
    Description: The discrepancy noted in radii obtained by the Baade-Wesselink method when different colors are used to determine the effective temperatures is explored. The discrepancy is found to be due to an inconsistency in the applied temperature-color calibrations. The assumption of the maximum likelihood method that beta (the effective temperature + 0.1 times the bolometric correction) is a linear function of the color is valid for the B-V and V-I colors, but not for the V-R colors. It is suggested that the errors introduced by the nonlinearity in the relation between beta and the V-R colors will produce radii which are too large. The radii derived from the V-B colors appear to be too small.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 343; 343-351
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 9
    Publication Date: 2018-06-08
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 10
    Publication Date: 2018-06-08
    Description: Near infrared images are presented of the Herbig-Haro 110 jet centered at the molecular hydrogen lines. The ratio of these lines provides a preliminary diagnostic of molecular gas excitation, which is expected from low velocity shocks and turbulent processes. It is suggested that the morphological properties of the molecular hydrogen emission are consistent with that of a boundary layer.
    Keywords: Astrophysics
    Type: The Astrophysical Journal
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...