Zobrazeno 1 - 10
of 35
pro vyhledávání: '"G. Erkeling"'
Publikováno v:
Planetary and Space Science. 144:49-70
In this paper, we present the results of our detailed study of morphology, topography, and age of the Deuteronilus contact that outlines Vastitas Borealis Formation (VBF) in the northern plains and the Isidis Planitia unit. The Deuteronilus contact r
Publikováno v:
Planetary and Space Science. 125:43-61
Images of Mars taken by spacecraft in the last few decades indicate that the landscape has changed and that current processes are continuously changing the surface. The modifications of the landscape are caused by exogenic processes including eolian
Autor:
G. Erkeling, H. Bernhardt, Ottaviano Ruesch, Dennis Reiss, Mikhail A. Ivanov, Harald Hiesinger
Publikováno v:
Icarus. 264:407-442
The Hellas basin on Mars is the second-largest topographically well-defined impact structure in the Solar System and has repeatedly been interpreted as a major sink of volcanic, glacio-fluvial and eolian materials. Based on established guidelines for
Publikováno v:
Icarus. 248:383-391
Utopia and Acidalia Planitiae show a set of similar morphologic features indicative of the presence of large reservoirs of water/mud in these regional topographic lows. The most important of these features are: (1) impact crater ejecta morphology tha
Autor:
Dennis Reiss, G. Erkeling, Ralf Jaumann, T. Heyer, Harald Hiesinger, D. Luesebrink, H. Bernhardt
Multi-temporal spacecraft observations are key to detect and understand surface changes and time-critical processes on Mars. Since the 1970s, the number of orbital observations of Mars has increased to over one million images. The observations have r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb3dcfc26b05d565e2aea1fbaba8a69d
https://elib.dlr.de/124615/
https://elib.dlr.de/124615/
Autor:
A. Petau, Ralf Jaumann, M. Sowe, E. Hauber, Daniela Tirsch, Harald Hiesinger, G. Erkeling, Laetitia Le Deit, Dennis Reiss, S. Adeli
Publikováno v:
Planetary and Space Science. 98:128-145
A study in context with the Helmholtz Alliance ‘Planetary Evolution and Life’ focused on the (temporary) existence of liquid water, and the likelihood that Mars has been or even is a habitable planet. Both geomorphological and mineralogical evide
Publikováno v:
Icarus. 228:121-140
Results of our detailed geological mapping and interpretation of the nature and relative and absolute model ages of units and structures in the SW portion of Utopia Planitia (20–45°N, 100–120°E) suggest the following. (1) The size–frequency d
Publikováno v:
Planetary and Space Science. 85:261-278
We present new insights into possible formation mechanisms and implications for previously identified landforms of putative glacio-fluvial origin along the southern rim of the Argyre basin on Mars. We compiled a detailed geomorphologic map of the stu
Autor:
Frank Fueten, Veronique Ansan, E. Kersten, Ernst Hauber, Jonas Bostelmann, M. Spiegel, Frank Scholten, Sebastian Walter, Alexander Dumke, T. Roatsch, Konrad Willner, G. Neukum, Patrick Pinet, Daniela Tirsch, S. van Gasselt, Dennis Reiss, Stephan Elgner, Patrick C. McGuire, R. Jaumann, Frank Preusker, Harald Hoffmann, N. M. Hoekzema, Volker Mertens, Juergen Oberst, K. Gwinner, Damien Loizeau, H. Hiesinger, Klaus-Dieter Matz, Robert Stesky, Ralph Schmidt, G. Erkeling, Marita Wählisch, A. Pasewaldt, Gregory Michael, Christian Heipke
Publikováno v:
Planetary and Space Science
Planetary and Space Science, Elsevier, 2016, 126, pp.93-138. ⟨10.1016/j.pss.2016.02.014⟩
Planetary and Space Science, Elsevier, 2016, 126, pp.93-138. ⟨10.1016/j.pss.2016.02.014⟩
The High Resolution Stereo Camera (HRSC) of ESA׳s Mars Express is designed to map and investigate the topography of Mars. The camera, in particular its Super Resolution Channel (SRC), also obtains images of Phobos and Deimos on a regular basis. As H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b8b76c71ebe0cf9e99f8f70f5ea8ed1
https://hal.archives-ouvertes.fr/hal-02306016
https://hal.archives-ouvertes.fr/hal-02306016
Publikováno v:
Icarus. 218:24-46
We have mapped the area of Isidis Planitia (1–27°N, 75–103°E) in order to assess the geologic history of this region using modern data sets such as MOLA topography and the high-resolution images provided by the HRSC, CTX, and HiRISE cameras. Re