Zobrazeno 1 - 10
of 40
pro vyhledávání: '"T. Hoogenboom"'
Publikováno v:
Meteoritics & Planetary Science. 55:2440-2460
Akademický článek
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Autor:
Kynan H.G. Hughson, Britney E. Schmidt, M. C. De Sanctis, H. Hiesinger, Thomas Platz, Katrin Krohn, Georgiana Y. Kramer, T. Hoogenboom, Christopher T. Russell, Simone Marchi, Jennifer E.C. Scully, Veronica J. Bray, Mark V. Sykes, L. Le Corre, Michael T. Bland, David P. O'Brien, Paul M. Schenk, Lucy A. McFadden, Julie Castillo-Rogez, Carol A. Raymond, Adrian Neesemann, Katharina A. Otto, Debra Buczkowski, S. Schroeder
Publikováno v:
Icarus. 359:114343
High-resolution mapping of Ceres, Vesta and the icy satellites of Saturn, Uranus and Pluto reveals a rich variety of well-preserved impact crater morphologies on these low gravity bodies. These objects provide a natural laboratory to study effects of
Publikováno v:
European Urology Supplements. 18:e1828
Autor:
T. Hoogenboom, V. Kavvadia, Paramaconi Rodriguez, Stanley C. S. Lai, Marc T. M. Koper, Matteo Duca
Publikováno v:
Journal of Electroanalytical Chemistry. 649:59-68
This paper reinvestigates the mechanism of HNO2 and NO2- reduction on polycrystalline platinum as a function of electrolyte pH and reactant concentration. Intermediates and/or reaction products were detected by means of various (combined) techniques:
Autor:
T. Hoogenboom, Suzanne E. Smrekar
Publikováno v:
Earth and Planetary Science Letters. 248:830-839
The northern lowlands cover approximately one-third of Mars' surface and are a fundamental part of the geologic evolution of Mars. We examine the admittance signature, the ratio of gravity to topography data in the spectral domain, for four regions i
Autor:
T. Hoogenboom, Gregory A. Houseman
Publikováno v:
Icarus. 180:292-307
In this study we explore the idea that coronae have formed on Venus as a result of gravitational (Rayleigh–Taylor) instability of the lithosphere. The lithosphere is represented by a system of stratified homogeneous viscous layers (low-density crus
Autor:
Christopher T. Russell, Roland Wagner, Frank Preusker, T. Hoogenboom, Jennifer E.C. Scully, Katrin Krohn, David A. Williams, Katharina A. Otto, Carol A. Raymond, Katrin Stephan, Ralf Jaumann, R. A. Yingst, Klaus-Dieter Matz, E. Kersten, Thomas Roatsch, Paul M. Schenk, Carle M. Pieters, Thomas Kneissl, Debra Buczkowski, M. C. De Sanctis, Nico Schmedemann, B. Garry
The Quadrangles Av-11 and Av-12 on Vesta are located at the northern rim of the giant Rheasilvia south polar impact basin. The primary geologic units in Av-11 and Av-12 include material from the Rheasilvia impact basin formation, smooth material and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c8491298917ebf7fb0b96d631f7b4d7
https://elib.dlr.de/90570/
https://elib.dlr.de/90570/
Publikováno v:
Journal of Geophysical Research. 115
[1] The two largest rift systems on Venus, Parga, and Hecate chasmata contain one third of all coronae. We map variations in elastic thickness and apparent depth of compensation (ADC) in these two regions using the admittance function for gravity and
Akademický článek
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