After more than ten years in orbit at Mars, the coverage from the High Resolution Stereo Camera (HRSC) on the European Space Agency’s Mars Express is sufficient to begin constructing mosaic products on a global scale. We describe our systematic processing procedure and, in particular, the technique used to bring images affected by atmospheric dust into visual consistency with the mosaic. We outline how the same method is used to produce a relative colour mosaic which shows local colour differences. We demonstrate the results and show that the techniques may also be applied to images from other orbital cameras
The pervasive Mars dust is continually transported between the surface and the atmosphere. When on t...
Mars Express is due to arrive in orbit around Mars during the last days of 2003. A primary task of i...
The Colour and Stereo Surface Science Imaging System (CaSSIS) of the ExoMars Trace Gas Orbiter retur...
AbstractAfter more than ten years in orbit at Mars, the coverage from the High Resolution Stereo Cam...
After more than ten years in orbit at Mars, the coverage from the High Resolution Stereo Camera (HRS...
A seamless mosaic has been constructed including a 3D terrain model at 50 m grid-spacing and a corre...
Since January 2004 the High Resolution Stereo Camera (HRSC) is mapping planet Mars. The multi-line s...
The High Resolution Stereo Camera (HRSC) of ESA’s Mars Express mission [1, 2] is still running nomin...
The European Mars Express mission was launched in June 2003 and sent into orbit around Mars. On boar...
International audienceThe High Resolution Stereo Camera (HRSC) of ESA's Mars Express is designed to ...
The Martian atmosphere often shows horizontal layers of haze up to altitudes of about 80 km. The Hig...
The European Mars Express mission was launched in June 2003 and sent into orbit around Mars. On boar...
For a systematic mapping of the Martian surface, the Mars Express orbiter is equipped with a multi-l...
The High Resolution Stereo Camera (HRSC) onboard the European Space Agency’s (ESA) Mars Express (MEX...
Mars rover colour vision typically employs multi-spectral imaging to generate natural-colour images ...
The pervasive Mars dust is continually transported between the surface and the atmosphere. When on t...
Mars Express is due to arrive in orbit around Mars during the last days of 2003. A primary task of i...
The Colour and Stereo Surface Science Imaging System (CaSSIS) of the ExoMars Trace Gas Orbiter retur...
AbstractAfter more than ten years in orbit at Mars, the coverage from the High Resolution Stereo Cam...
After more than ten years in orbit at Mars, the coverage from the High Resolution Stereo Camera (HRS...
A seamless mosaic has been constructed including a 3D terrain model at 50 m grid-spacing and a corre...
Since January 2004 the High Resolution Stereo Camera (HRSC) is mapping planet Mars. The multi-line s...
The High Resolution Stereo Camera (HRSC) of ESA’s Mars Express mission [1, 2] is still running nomin...
The European Mars Express mission was launched in June 2003 and sent into orbit around Mars. On boar...
International audienceThe High Resolution Stereo Camera (HRSC) of ESA's Mars Express is designed to ...
The Martian atmosphere often shows horizontal layers of haze up to altitudes of about 80 km. The Hig...
The European Mars Express mission was launched in June 2003 and sent into orbit around Mars. On boar...
For a systematic mapping of the Martian surface, the Mars Express orbiter is equipped with a multi-l...
The High Resolution Stereo Camera (HRSC) onboard the European Space Agency’s (ESA) Mars Express (MEX...
Mars rover colour vision typically employs multi-spectral imaging to generate natural-colour images ...
The pervasive Mars dust is continually transported between the surface and the atmosphere. When on t...
Mars Express is due to arrive in orbit around Mars during the last days of 2003. A primary task of i...
The Colour and Stereo Surface Science Imaging System (CaSSIS) of the ExoMars Trace Gas Orbiter retur...