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.
| Line of Cones and Associated Flows in Arsia Sulci: PSP_007603_1770 ESP_036718_1770 (Interval in Earth days: 2269) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.83 | 231. | 8.18 | -17.6 | 47.1 | 57.8 |
| Dark Dune-Like Forms in Southern Melas Chasma: PSP_007522_1685 ESP_025666_1685 (Interval in Earth days: 1414) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 284. | 0.94 | -27.7 | 51.1 | 56.6 |
| Chasma Borealis: PSP_007020_2580 PSP_007178_2580 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.78 | 292. | 0 | 12.81 | 69.8 | 67.1 |
| Lava Flow Contacts in Eastern Elysium Planitia: PSP_007170_1820 PSP_007381_1820 (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 | 2.197 | 174. | 13.9 | -6.48 | 40.3 | 43.9 |
| Central Peak of Unnamed Crater within the Medusae Fossae Formation: PSP_007870_1830 PSP_009228_1830 (Interval in Earth days: 106) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.031 | 140. | 4.36 | -20.5 | 47.0 | 55.2 |
| Light-Toned Outcrops Exhumed From Dark Material in Arabia Terra: PSP_008139_1905 PSP_009576_1905 (Interval in Earth days: 112) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.54 | 355. | -7.9 | 17.40 | 46.6 | 49.4 |
| Central Peak Region of Canso Crater: PSP_007139_2015 ESP_085442_2015 (Interval in Earth days: 6101) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.34 | 299. | -1.5 | -10.2 | 39.3 | 44.2 |
| Crater Interior with Light-Toned Rock and Curvilinear Ridge Features: PSP_007465_1595 ESP_085755_1595 (Interval in Earth days: 6100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.2 | 42.9 | -4.0 | -22.9 | 56.2 | 44.2 |
| 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 |
| Northwest Hellas Basin Landforms: PSP_007636_1400 ESP_016075_1400 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 55.9 | 0.23 | -23.1 | 71.3 | 67.4 |
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