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.
| Lava-Coated Craters : ESP_052347_1860 ESP_052993_1860 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.126 | 148. | -0.8 | 19.68 | 45.4 | 46.5 |
| Unusual Hills West of Olympus Mons : ESP_052015_1950 ESP_052160_1950 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.88 | 211. | 3.55 | 20.46 | 39.7 | 39.1 |
| Channel in Phlegra Montes : ESP_052254_2195 ESP_052544_2195 (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 | 39.14 | 164. | -7.5 | 7.795 | 39.7 | 38.3 |
| Candidate Red Dragon Landing Site in Arcadia Planitia : ESP_052279_2210 ESP_052345_2210 (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 | 40.64 | 200. | -0.9 | -17.9 | 39.4 | 40.8 |
| Well-Preserved Crater North of Hellas Planitia : ESP_052218_1635 ESP_060183_1635 (Interval in Earth days: 620) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.1 | 74.3 | -6.3 | 5.878 | 58.1 | 48.6 |
| Winding Channel : ESP_052236_2080 ESP_052447_2080 (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 | 27.74 | 296. | 7.99 | -4.60 | 37.8 | 39.3 |
| Candidate Recent Impact Site : ESP_052124_1860 ESP_052546_1860 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.926 | 117. | 1.42 | -23.5 | 44.0 | 48.2 |
| Fan Material at an Alcove on Southwestern Aeolis Mons : ESP_052242_1745 ESP_063319_1745 (Interval in Earth days: 863) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.48 | 137. | -1.7 | 14.83 | 51.1 | 56.0 |
| Megabreccia at Contact in Northeast Syrtis Major Region : ESP_052165_1975 ESP_052231_1975 (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 | 17.33 | 76.6 | 1.19 | -20.9 | 40.0 | 42.1 |
| Sinuous Ridge : ESP_052275_2235 ESP_052552_2235 (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 | 43.39 | 309. | 0.18 | -24.4 | 39.9 | 41.9 |
Page 323 of 891 (8,901 images) | |||||