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.
| Light-Toned Layered Deposits in Valles Marineris : ESP_043731_1655 ESP_043665_1655 (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 | -14.1 | 298. | 7.33 | 27.69 | 58.7 | 57.1 |
| Northern Plains Crater Modification : ESP_043549_2265 ESP_043615_2265 (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 | 45.99 | 220. | -5.7 | -18.9 | 41.7 | 42.7 |
| Pit Near Elysium Mons : ESP_043763_2100 ESP_071022_2100 (Interval in Earth days: 2124) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.69 | 139. | 10.5 | -3.75 | 38.7 | 47.6 |
| Gullied Crater in Tempe Terra : ESP_043705_2225 ESP_043771_2225 (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 | 41.98 | 282. | -5.5 | -19.7 | 40.5 | 41.7 |
| Smooth and Knobby Terrain in Lyot Crater Ejecta : ESP_043622_2330 ESP_043754_2330 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 52.55 | 27.4 | -8.9 | -29.3 | 43.9 | 45.5 |
| Kasei Valles Lava Flow : ESP_043784_2040 ESP_044760_2040 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.88 | 287. | 7.53 | -25.5 | 40.0 | 44.1 |
| Valley Intersecting Crater in Nepenthes Region : ESP_043685_1895 ESP_044806_1895 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.196 | 112. | -4.0 | -22.1 | 45.7 | 48.5 |
| Well-Preserved Impact Crater in Meridiani Planum : ESP_043557_1770 ESP_044335_1770 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.99 | 8.83 | -7.2 | 7.52 | 51.8 | 52.9 |
| Mamers Valles Source : ESP_043794_2210 ESP_044084_2210 (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 | 40.59 | 12.4 | 0.68 | 25.94 | 39.7 | 37.3 |
| Meander in Channel in Cydonia Mensae : ESP_043623_2160 ESP_051126_2160 (Interval in Earth days: 585) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.86 | 1.35 | 1.88 | -15.6 | 39.4 | 42.2 |
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