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 Rock Exposures: PSP_007101_1730 ESP_019311_1730 (Interval in Earth days: 952) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.99 | 260. | -7.9 | 3.361 | 44.7 | 56.7 |
| Unmantled Central Uplift Feature in Unnamed Crater: PSP_007526_1435 PSP_010875_1435 (Interval in Earth days: 261) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.4 | 178. | 4.32 | -6.88 | 67.4 | 70.7 |
| Hellas Planitia: PSP_007715_1420 ESP_016022_1420 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.4 | 57.6 | 8.36 | 23.98 | 70.4 | 62.4 |
| Well-Peserved Large Crater with Central Peak and Pit: PSP_007366_1360 ESP_024732_1360 (Interval in Earth days: 1353) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.4 | 229. | 2.46 | -27.4 | 70.5 | 67.3 |
| Fault Relays in the Cerberus Fossae: PSP_007645_1885 PSP_007856_1885 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.465 | 164. | -5.5 | -23.3 | 43.9 | 46.8 |
| Light-Toned Layered Rock Outcrops in Southern Mid-Latitude Crater: PSP_008070_1465 PSP_009151_1465 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.2 | 84.4 | -2.9 | 11.17 | 71.8 | 76.2 |
| Fading Rayed Crater in Daedalum Planum: PSP_007735_1570 ESP_028345_1570 (Interval in Earth days: 1606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 230. | 2.03 | -10.9 | 60.9 | 63.5 |
| Cratered Cones in Isidis Planitia: PSP_007872_1900 PSP_009586_1900 (Interval in Earth days: 134) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.820 | 85.7 | -6.6 | -23.4 | 45.1 | 52.9 |
| Debris Flows on Mars: PSP_007033_1445 ESP_016197_1445 (Interval in Earth days: 714) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.9 | 321. | -6.8 | 8.328 | 59.9 | 64.1 |
| Floor and Central Uplift of Mazamba Crater in Thaumasia Planum: PSP_007100_1520 ESP_033248_1520 (Interval in Earth days: 2038) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 290. | -1.6 | -23.6 | 55.6 | 51.8 |
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