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05.02.2004
HRSC Press Release #015 - Canyons (orbit 0018)
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The first anaglyph-picture has been calculated from the nadir and stereo channels of the HRSC. The pictures were taken in orbit 18 on 14 January 2004 from a height of 275 km and are located on Mars at the equator north of Valles Marineris between 1° South to 2.5° North and 323° East. The area is 50 km across, has a resolution of 12 m per pixel, and shows mesas and cliffs as well as flow features which indicate erosion by the action of flowing water. The landscape is seen in a vertical view, North is at right.
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The second anaglyph-picture has been calculated from the nadir and stereo channels of the HRSC. The pictures were taken in orbit 18 on 14 January 2004 from a height of 275 km and are located on Mars north of Valles Marineris between 5° to 10° North and 323° East. The area is 50 km across, has a resolution of 12 m per pixel, and shows mesas and cliffs indicating erosion by the action of flowing water. The landscape is seen in a vertical view, North is at right.
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Die Farbansichten wurden aus dem senkrecht blickenden Nadirkanal und den Farbkanälen erstellt, die Schrägansicht wurde aus den Stereokanälen der HRSC berechnet. Die Anaglyphen werden aus dem Nadirkanal und einem Stereokanal abgeleitet. Die schwarzweißen Detailaufnahmen wurden dem Nadirkanal entnommen, der von allen Kanälen die höchste Auflösung zur Verfügung stellt.
The colour scenes have been derived from the three HRSC-colour channels and the nadir channel. The
perspective views have been calculated from the digital terrain model derived from the
stereo channels. The anaglyph image was calculated from the nadir and one stereo channel.
The black and white high resolution images were derived form the nadir channel which provides the
highest detail of all channels.
Das Kameraexperiment HRSC auf der Mission Mars Express der
Europäischen Weltraumorganisation ESA wird vom Principal Investigator Prof. Dr.
Gerhard Neukum (Freie Universität Berlin), der auch die technische Konzeption der
hochauflösenden Stereokamera entworfen hatte, geleitet. Das
Wissenschaftsteam besteht aus 40 Co-Investigatoren aus 33 Institutionen und zehn
Nationen. Die Kamera wurde am Deutschen Zentrum für Luft- und Raumfahrt (DLR) unter der
Leitung des Principal Investigators (PI) G. Neukum entwickelt und in Kooperation mit
industriellen Partnern gebaut (EADS Astrium, Lewicki Microelectronic GmbH und Jena
-Optronik GmbH). Sie wird vom DLR -Institut für Planetenforschung in Berlin-Adlershof
betrieben. Die systematische Prozessierung der Daten erfolgt am DLR. Die Darstellungen
wurden vom Institut für Geologische Wissenschaften der FU Berlin in Zusammenarbeit
mit dem DLR-Institut für Planetenforschung erstellt.
The High Resolution Stereo Camera (HRSC) experiment on the ESA Mars Express Mission is led by the
Principal Investigator (PI) Prof. Dr. Gerhard Neukum who also designed the camera technically. The
science team of the experiment consists of 40 Co-Investigators from 33 institutions and 10 nations.
The camera was developed at the German
Aerospace Center (DLR) under
the leadership of the PI G. Neukum and built in cooperation with industrial partners (EADS
Astrium, Lewicki Microelectronic GmbH and Jena-Optronik GmbH). The experiment on Mars Express
is operated by the DLR Institute of Planetary Research, through ESA/ESOC. The systematic
processing of the HRSC image data is carried out at DLR. The scenes shown here were created
by the PI-group at the Institute for Geological Sciences of the Freie Universitaet Berlin in
cooperation with the German Aerospace Center (DLR), Institute of Planetary Research, Berlin.
Download
hochaufgelöste Bilddaten / high resolution image data
| RGB Farbbild #1: |
| RGB Farbbild #2: |
| Rot-Cyan Anaglyphe #1: |
| Rot-Cyan Anaglyphe #2: |
© Copyright: ESA/DLR/FU Berlin (G. Neukum)
