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.
| Possible Terraced Crater in Arcadia Planitia: ESP_034319_2260 ESP_034754_2260 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.67 | 198. | 3.45 | 23.42 | 42.8 | 40.0 |
| Meander in Central Channel in Nanedi Valles: ESP_034236_1855 ESP_035792_1855 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.183 | 310. | 3.71 | -19.7 | 44.7 | 53.6 |
| Light-Toned Stratified Materials in Melas Chasma: ESP_034250_1670 ESP_035450_1670 (Interval in Earth days: 93) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.8 | 289. | 12.9 | -23.9 | 53.7 | 63.6 |
| Crater-Related Pitted Materials in 8-Kilometer Diameter Hellas Region Crater: ESP_034297_1380 ESP_034363_1380 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.9 | 91.6 | 1.75 | -17.4 | 75.1 | 76.9 |
| Mesa in Olympica Fossae: ESP_034146_2050 ESP_034436_2050 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.78 | 246. | -8.3 | 18.70 | 40.6 | 39.1 |
| Outflow Channel Features Associated with Small Chaotic Terrain: ESP_034355_1770 ESP_034922_1770 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.88 | 302. | 6.96 | -7.21 | 49.3 | 54.3 |
| North Polar Residual Cap: ESP_034369_2690 ESP_034526_2690 (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 | 89.00 | 280. | -27. | -22.1 | 69.1 | 67.5 |
| Channel System in Tharsis Region: ESP_034489_2005 ESP_034779_2005 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.24 | 241. | -3.1 | 18.59 | 41.9 | 41.3 |
| Flows Near Echus Chasma: ESP_034158_1865 ESP_037270_1865 (Interval in Earth days: 242) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.245 | 279. | 6.61 | -18.3 | 43.4 | 56.1 |
| Northern Plains Features: ESP_034200_2335 ESP_034266_2335 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.02 | 205. | 4.92 | -6.54 | 46.1 | 46.6 |
Page 477 of 877 (8,766 images) | |||||