Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| A Triple-Crater in Elysium Planitia: ESP_039147_1940 ESP_039292_1940 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.78 | 167. | -3.4 | 8.285 | 61.2 | 59.7 |
| Strange Flow: Landslide, Impact Melt or Lava?: ESP_039117_1745 ESP_039539_1745 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.45 | 267. | 14.2 | -4.61 | 51.1 | 48.1 |
| Light-Toned Layered Deposits along Western Ladon Valles Basin Floor: ESP_039194_1605 ESP_047541_1605 (Interval in Earth days: 650) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.4 | 328. | -12. | -27.2 | 48.3 | 49.9 |
| Junctions between Wide Channels and Narrow Channels: ESP_039174_1730 ESP_066167_1730 (Interval in Earth days: 2104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.70 | 151. | 5.09 | 22.54 | 50.8 | 45.8 |
| Margin of Pedestal Crater in Malea Planum: ESP_039126_1215 ESP_039627_1215 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -58.3 | 31.4 | -5.5 | 7.724 | 53.2 | 46.8 |
| Landforms of Eastern Hydraotes Chaos: ESP_039128_1800 ESP_039761_1800 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.16 | 327. | 1.77 | -15.4 | 54.0 | 48.9 |
| Candidate ExoMars Landing Site: ESP_039036_1925 ESP_039458_1925 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.14 | 315. | 26.1 | 6.489 | 58.6 | 57.6 |
| Flow Features in Arimanes Rupes Region East of Mangala Valles: ESP_038908_1670 ESP_039396_1670 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 212. | 26.6 | -4.87 | 49.7 | 47.0 |
| Well-Preserved 2-Kilometer Crater over Bedrock: ESP_039138_1545 ESP_046852_1545 (Interval in Earth days: 601) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.4 | 58.0 | -6.0 | 9.496 | 47.7 | 53.8 |
| Pavonis Mons: ESP_039131_1830 ESP_039342_1830 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.876 | 244. | 6.87 | -5.46 | 55.0 | 54.2 |
Page 442 of 896 (8,955 images) | |||||