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 Sulfate-Rich Terrain in Northeast Syrtis Major Region: ESP_042750_1970 ESP_043172_1970 (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 | 16.63 | 77.4 | 7.00 | -9.18 | 39.0 | 41.7 |
| Concentric Crater Fill: ESP_042931_2315 ESP_043208_2315 (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 | 51.07 | 171. | -3.0 | -19.5 | 46.1 | 45.9 |
| Small Buttes and Dunes in Meridiani Planum: ESP_042951_1820 ESP_043017_1820 (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 | 2.207 | 352. | -4.3 | -26.0 | 45.2 | 47.4 |
| Candidate ExoMars Landing Site in Aram Dorsum: ESP_042872_1880 ESP_051298_1880 (Interval in Earth days: 656) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.875 | 348. | 2.36 | -8.33 | 42.0 | 37.9 |
| Expanded Secondary Craters in Arcadia Planitia: ESP_042824_2315 ESP_044103_2315 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.37 | 212. | -2.1 | 15.43 | 46.8 | 40.6 |
| Pits and Troughs in Tempe Terra: ESP_042821_2140 ESP_069302_2140 (Interval in Earth days: 2063) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.51 | 297. | 2.64 | -6.72 | 40.1 | 48.1 |
| Terrain Northwest of Elysium Mons: ESP_043025_2095 ESP_080042_2095 (Interval in Earth days: 2884) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.04 | 128. | -3.3 | 9.461 | 39.7 | 45.9 |
| Daedalia Planum Lava Flows: ESP_042718_1545 ESP_043008_1545 (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 | -25.1 | 236. | 2.74 | 28.48 | 58.1 | 59.7 |
| Zir Crater in Chryse Planitia: ESP_043097_1985 ESP_043519_1985 (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 | 18.53 | 323. | 6.46 | -4.78 | 39.8 | 41.9 |
| Nili Patera Dunes: ESP_042790_1890 ESP_042144_1890 (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 | 8.797 | 67.1 | -3.4 | -28.2 | 41.7 | 40.5 |
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