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 Phyllosilicate Detection in a Small Crater Near Gale Crater Rim : ESP_044660_1740 ESP_045504_1740 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.07 | 136. | 12.5 | 28.31 | 54.3 | 50.9 |
| Northwestern Discontinuous Ejecta and Rays of Gratteri Crater : ESP_044737_1625 ESP_044394_1625 (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 | -17.5 | 199. | -24. | 11.61 | 64.0 | 62.2 |
| Crater with Thin Ejecta in Ismeniae Fossae Region : ESP_044769_2235 ESP_062927_2235 (Interval in Earth days: 1415) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.96 | 35.8 | 2.76 | -5.40 | 41.1 | 47.8 |
| North Polar Dunes : ESP_044851_2580 ESP_044376_2580 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.78 | 307. | -3.1 | 10.62 | 57.1 | 54.5 |
| Linear Ridge Features and Possible Mounds in Lyot Crater : ESP_044967_2300 ESP_045165_2300 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.48 | 29.5 | 6.01 | -25.0 | 43.3 | 47.5 |
| Candidate Landing Site for 2020 Mission in Hypanis Valles Delta : ESP_044970_1920 ESP_044693_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 | 11.92 | 314. | -7.7 | 6.83 | 46.3 | 45.1 |
| Multiple Geomorphic and Geologic Units in Southern Meridiani Planum : ESP_044665_1785 ESP_069445_1785 (Interval in Earth days: 1931) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.58 | 0.32 | 8.50 | -23.2 | 51.9 | 57.4 |
| Crater on Lobate Apron : ESP_044690_2225 ESP_045191_2225 (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 | 42.24 | 33.6 | -6.9 | 27.01 | 41.5 | 41.0 |
| Atypical Landform among Dunes in Polar Erg : ESP_044917_2575 ESP_044864_2575 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.54 | 307. | -7.0 | 8.026 | 57.6 | 56.4 |
| Terraced Crater in Amazonis Planitia : ESP_044697_2090 ESP_044974_2090 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.64 | 203. | -2.8 | -14.9 | 41.1 | 42.9 |
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