High Resolution Stereo Camera
High Resolution Stereo Camera (HRSC) is a camera experiment on Mars Express. A version for Earth called HRSC-AX was also developed, as was a version for Mars 96. It has four main parts: camera head, super resolution channel, instrument frame, and digital unit. At an altitude of 250 km from Mars, SRC can produce images with a resolution of 2.3 meters/pixel of 2.35 km square Mars terrain. It has 9 channels and can produce digital terrain models. A typical image from HRSC of Mars has a resolution ranging from 12.5 for nadir (directly down) to 25 m/pixel for the furthest off-nadir shots, which can be up to 18.9 degrees. By 2012, about 61.5% of the surface of Mars was mapped at a resolution of at least 20 meters per pixel by the Mars Express mission using this camera. Another area of study is repeat imaging, to allow the study of dynamic processes on Mars. Another trick is to make short videos of the Mars surface by taking advantage of the pushbroom nature of the detector. Each section is slightly offset for a different color, but when combined, every view is used to make a short animation. By the start of 2015, about 70% of Mars had been imaged at resolutions greater than 20 m per pixel, and 97% at resolutions of least 60 m per pixel.
High Resolution Stereo Camera (HRSC) is a camera experiment on Mars Express.[1] A version for Earth called HRSC-AX was also developed, as was a version for Mars 96.[1] It has four main parts: camera head, super resolution channel, instrument frame, and digital unit.[1] At an altitude of 250 km from Mars, SRC can produce images with a resolution of 2.3 meters/pixel of 2.35 km square Mars terrain.[1] It has 9 channels and can produce digital terrain models.[1] A typical image from HRSC of Mars has a resolution ranging from 12.5 for nadir (directly down) to 25 m/pixel for the furthest off-nadir shots, which can be up to 18.9 degrees.[2]
By 2012, about 61.5% of the surface of Mars was mapped at a resolution of at least 20 meters per pixel by the Mars Express mission using this camera.[3] Another area of study is repeat imaging, to allow the study of dynamic processes on Mars.[2][4] Another trick is to make short videos of the Mars surface by taking advantage of the pushbroom nature of the detector. Each section is slightly offset for a different color, but when combined, every view is used to make a short animation.[5]
By the start of 2015, about 70% of Mars had been imaged at resolutions greater than 20 m per pixel, and 97% at resolutions of least 60 m per pixel.[6]
Example observation
[edit]Orcus Patera, imaged by the HRSC:
See also
[edit]- Trace Gas Orbiter (next ESA Mars orbiter, arrived 2016)
References
[edit]- ^ a b c d e DLR – HRSC on Mars Express Archived 2012-01-17 at the Wayback Machine
- ^ a b "High-resolution repeat imaging allows detecting dynamic surface processes on Mars".
- ^ ESA -Mapping Mars
- ^ Sidiropoulos, P.; Muller, J.-P. (2015). "On the status of orbital high-resolution repeat imaging of Mars for the observation of dynamic surface processes" (PDF). Planetary and Space Science. 117: 207–222. Bibcode:2015P&SS..117..207S. doi:10.1016/j.pss.2015.06.017.
- ^ TPS – Capturing Martian Weather in Motion – November 4, 2016
- ^ THE HIGH RESOLUTION STEREO CAMERA (HRSC): STATUS AND FACTS (2015)
External links
[edit]
- ESA – High Resolution Stereo Camera
- Aeolis Mons (Mount Sharp) and Gale – Image/HRSCview Archived 2017-08-07 at the Wayback Machine
- Aeolis Mons (Mount Sharp) – HRSCview Archived 2016-08-05 at the Wayback Machine (oblique view looking east)
- HRSC + Phobos Archived 2013-11-11 at the Wayback Machine (with SRC shots overlaid)
- HRSC Press release archive (2004–2012)
- HRSC with SRC of Victoria Crater and area near Opportunity rover's landing site Archived 2016-11-13 at the Wayback Machine
- Clouds in Nilokeras Scopulus Archived 2016-11-13 at the Wayback Machine
- TPS – Capturing Martian Weather in Motion – November 4, 2016
- THE HIGH RESOLUTION STEREO CAMERA (HRSC): STATUS AND FACTS (2015) (Includes graph of cumulative surface coverage by resolution, up to 2015)
| Spacecraft |
|  |
|---|---|---|
| Instruments |
| |
| Related spacecraft |
| |