Frank Scholten mainly focuses on Comet, Astrophysics, Astrobiology, Remote sensing and Astronomy. His work deals with themes such as Touchdown, Surface and Trajectory, which intersect with Comet. His Astrophysics research includes elements of Stratification and Debris.
In his research, Infrared is intimately related to Spacecraft, which falls under the overarching field of Astrobiology. His Remote sensing study combines topics in areas such as Orientation, Pixel, High Resolution Stereo Camera and Terrain. His Astronomy research is multidisciplinary, incorporating perspectives in Spectrophotometry and Venus.
His primary scientific interests are in Remote sensing, Comet, Astrobiology, Mars Exploration Program and High Resolution Stereo Camera. His Remote sensing research is multidisciplinary, relying on both Pixel, Orbiter, Terrain and Geodesy. Astrophysics and Astronomy are inherently bound to his Comet studies.
His studies deal with areas such as Spectrophotometry and Spectral slope as well as Astrophysics. Astrobiology and Spacecraft are frequently intertwined in his study. His research integrates issues of Image resolution, Planet and Stereo imaging in his study of High Resolution Stereo Camera.
Frank Scholten mostly deals with Comet, Astrophysics, Astronomy, Osiris and Asteroid. His Comet study is associated with Astrobiology. His Astrophysics research incorporates themes from Brightness, Infrared and Outflow.
His work on Southern Hemisphere, Solar System and Outgassing as part of general Astronomy study is frequently linked to Sublimation, bridging the gap between disciplines. In Surface, Frank Scholten works on issues like Thermal model, which are connected to Remote sensing. His Remote sensing research includes themes of Orientation, Computer vision and High Resolution Stereo Camera.
His primary areas of investigation include Comet, Astrophysics, Astronomy, Astrobiology and Surface. He has researched Comet in several fields, including Thermal, Computer graphics and Erosion. His Astrophysics research integrates issues from Brightness and Infrared.
Frank Scholten regularly ties together related areas like Pixel in his Astronomy studies. His Astrobiology research is multidisciplinary, incorporating elements of Matrix and Weathering. Frank Scholten combines subjects such as Subdivision, Formation and evolution of the Solar System, Meteorite and Asteroid with his study of Surface.
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On the nucleus structure and activity of comet 67P/Churyumov-Gerasimenko
Holger Sierks;Cesare Barbieri;Philippe L. Lamy;Rafael Rodrigo;Rafael Rodrigo.
The high-resolution stereo camera (HRSC) experiment on Mars Express: Instrument aspects and experiment conduct from interplanetary cruise through the nominal mission
R. Jaumann;G. Neukum;T. Behnke;T.C. Duxbury.
Planetary and Space Science (2007)
The morphological diversity of comet 67P/Churyumov-Gerasimenko
Nicolas Thomas;Holger Sierks;Cesare Barbieri;Philippe L. Lamy.
The landing(s) of Philae and inferences about comet surface mechanical properties
Jens Biele;Stephan Ulamec;Michael Maibaum;Reinhard Roll.
A homogeneous nucleus for comet 67P/Churyumov-Gerasimenko from its gravity field
M Pätzold;T. Andert;Matthias Hahn;S.W. Asmar.
GLD100: The near-global lunar 100 m raster DTM from LROC WAC stereo image data
Frank Scholten;J. Oberst;J. Oberst;K.-D. Matz;Thomas Roatsch.
Journal of Geophysical Research (2012)
Vesta’s Shape and Morphology
R. Jaumann;R. Jaumann;David Williams;D. L. Buczkowski;R. A. Yingst.
Shape model, reference system definition, and cartographic mapping standards for comet 67P/Churyumov-Gerasimenko Stereo-photogrammetric analysis of Rosetta/OSIRIS image data
Frank Preusker;F. Scholten;K.-D. Matz;Thomas Roatsch.
Astronomy and Astrophysics (2015)
Spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from the OSIRIS instrument onboard the ROSETTA spacecraft
S. Fornasier;P. H. Hasselmann;M. A. Barucci;C. Feller.
Astronomy and Astrophysics (2015)
Images of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar System
H. Sierks;P. Lamy;Cesare Barbieri;D. Koschny.
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