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This HRSC mosaic shows the central region of Tiu Vallis. The mosaic consists of ten single HRSC orbits and extends over 379 km (N-S) und 298 km (E-W). The total aerial coverage is about 113000 km². The HRSC-DTM has a resolution of 100 m/Pixel whereas the nadir mosaic was processed at a resolution of 12.5 m/Pixel. The scenes shown here were created at the Department of Planetary Sciences and Remote Sensing, at the Institute of Geological Sciences of the Freie Universitaet Berlin.
Link to HRSCView:
: Selected single orbit parameters
| Orbit | 0018 | 1143 | 1154 | 1991 | 2002 | 2013 | 2024 | 2035 | 2046 | 5156 |
| Sequence | 0 | 0 | 1 | 0 | 1 | 1 | 1 | 0 | 0 | 0 |
| Centre Longitude [°] | 36.84 | 34.87 | 35.82 | 32.29 | 33.27 | 34.18 | 35.03 | 35.87 | 36.7 | 35.91 |
| Centre Latitude [°] |
-1.56 | 18.81 | 18.55 | 7.74 | 7.68 | 3.54 | 3.26 | 7.98 | 14.51 | 8.45 |
| Solar Longitude [°] |
333.07 | 126.23 | 127.7 | 261.64 | 263.59 | 265.53 | 267.47 | 269.42 | 271.35 | 13.85 |
| Image Date |
14.01. 2004 |
08.12. 2004 |
11.12. 2004 |
03.08. 2005 |
06.08. 2005 |
09.08. 2005 |
12.08. 2005 |
15.08. 2005 |
18.08. 2005 |
07.01. 2008 |
| Scaled Height [km] |
1663 | 799.7 | 799.2 | 1583.7 | 1588 | 1105.9 | 1195.8 | 1708.8 | 305.1 | 535.3 |
| Scaled Width [km] |
68.4 | 67 | 79.9 | 70.3 | 71 | 66.4 | 67.9 | 80.8 | 72.8 | 70.7 |
| Scaled Pixel Width [km] |
0.0125 | 0.0125 | 0.0125 | 0.0125 | 0.0125 | 0.0125 | 0.0125 | 0.0125 | 0.0125 | 0.0125 |
| Best Ground Resolution [km] |
0.011 | 0.0119 | 0.0123 | 0.012 | 0.012 | 0.0119 | 0.0118 | 0.0118 | 0.0132 | 0.013 |
| Phase Angle [°] |
31.11 | 30.59 | 9.18 | 67.87 | 65.82 | 57.97 | 56.23 | 61.87 | 65.57 | 59.14 |
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.
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hochaufgelöste Bilddaten / high resolution image data
© Copyright: ESA/DLR/FU Berlin (G. Neukum)
