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.
| Depression in Osuga Valles: ESP_069697_1650 ESP_078611_1650 (Interval in Earth days: 694) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.6 | 322. | 0.25 | -16.0 | 64.8 | 61.5 |
| Xanthe Dorsa: ESP_069987_2245 ESP_070277_2245 (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 | 44.03 | 317. | -7.5 | 5.319 | 48.4 | 46.5 |
| Light-Toned Layered Deposits in Ladon Valles Basin: ESP_069301_1595 ESP_069367_1595 (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 | -20.2 | 329. | 7.95 | -6.97 | 63.1 | 64.9 |
| Alluvial Fans in Ganges Chasma: ESP_069341_1715 ESP_069684_1715 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.37 | 317. | 3.92 | -6.68 | 57.4 | 61.7 |
| Central Peak of Crater in Solis Planum: ESP_069329_1500 ESP_071465_1500 (Interval in Earth days: 166) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.8 | 288. | -6.9 | 29.58 | 70.2 | 72.9 |
| Layers in Candor Chasma: ESP_069487_1725 ESP_069553_1725 (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 | -7.49 | 292. | 8.60 | -6.93 | 58.2 | 60.0 |
| Candidate M2020 Perseverance Entry Vehicle Ballast Impacts Zone: ESP_069231_1990 ESP_088852_1990 (Interval in Earth days: 1529) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.92 | 76.2 | -1.3 | 24.39 | 47.8 | 45.9 |
| Alluvial Fans in Juventae Chasma: ESP_069434_1750 ESP_069856_1750 (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 | -4.92 | 298. | 0.20 | 11.95 | 57.0 | 59.4 |
| Layers in Crater North of Hellas Planitia: ESP_069495_1525 ESP_078475_1525 (Interval in Earth days: 700) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.2 | 76.5 | 5.77 | -5.68 | 69.9 | 67.9 |
| Rough Terrain in Xanthe Terra: ESP_069552_1920 ESP_069618_1920 (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 | 11.92 | 315. | 7.8 | -6.51 | 50.7 | 52.2 |
Page 209 of 913 (9,124 images) | |||||