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.
| Candidate Impact Site Formed between September 2008 and Dec 2015 : ESP_045956_1855 ESP_064272_1855 (Interval in Earth days: 1427) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.372 | 37.3 | -4.8 | 8.328 | 49.5 | 56.4 |
| Channel in Maadim Vallis : ESP_045951_1560 ESP_046162_1560 (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 | -23.5 | 176. | 7.72 | -1.89 | 60.0 | 59.2 |
| Fractures in Utopia Planitia : ESP_046151_2140 ESP_046573_2140 (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 | 33.84 | 108. | 4.82 | -6.29 | 51.2 | 57.7 |
| Streamlined Shape in Marte Vallis : ESP_045911_1995 ESP_046412_1995 (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 | 19.27 | 184. | -4.7 | 13.68 | 47.6 | 50.2 |
| Pits and Lava in Amazonis Planitia : ESP_045818_1965 ESP_046240_1965 (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 | 16.13 | 202. | 5.08 | -13.5 | 46.3 | 50.8 |
| Ridges in Cydonia Region : ESP_045918_2160 ESP_046419_2160 (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 | 35.61 | 351. | -5.8 | 9.679 | 49.6 | 55.0 |
| Crater with Blocky Interior in Marte Vallis : ESP_045977_1920 ESP_046267_1920 (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 | 11.83 | 183. | -6.5 | 20.42 | 48.6 | 48.0 |
| Small Channel in Wall of Orson Welles Crater : ESP_046025_1790 ESP_071464_1790 (Interval in Earth days: 1982) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.20 | 314. | -7.0 | 7.433 | 51.4 | 57.3 |
| Noachis Terra : ESP_045905_1425 ESP_069076_1425 (Interval in Earth days: 1805) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 355. | -2.1 | -14.8 | 68.8 | 71.7 |
| Candidate Landing Site for 2020 Mission in Jezero Crater : ESP_045994_1985 ESP_046060_1985 (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 | 18.42 | 77.4 | 3.48 | -18.2 | 47.5 | 49.9 |
Page 360 of 877 (8,765 images) | |||||