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.
| Central Peak of Large 40-Kilometer Diameter Crater: PSP_007592_1995 ESP_045595_1995 (Interval in Earth days: 2961) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.25 | 169. | -0.9 | 19.06 | 40.8 | 43.5 |
| Distal End of Lethe Vallis: PSP_007263_1845 PSP_007553_1845 (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 | 4.500 | 156. | -7.8 | 5.828 | 42.2 | 43.6 |
| Crater with Multiple Gully Orientations: PSP_007001_2200 PSP_007937_2200 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.48 | 105. | -8.6 | 6.751 | 45.7 | 41.3 |
| Gullies as Seen in MOC Image M02-02681: PSP_007213_1400 ESP_042618_1400 (Interval in Earth days: 2759) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 86.3 | 2.71 | 26.46 | 65.4 | 65.6 |
| 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 |
| Well-Exposed Scarp of Noachian Phyllosilicates Along Nili Fossae: PSP_007200_2005 ESP_016153_2005 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.03 | 73.6 | 1.53 | 26.79 | 39.1 | 37.1 |
| Well-Preserved 15-Kilometer Diameter Crater Near Nili Fossae: PSP_007912_2030 ESP_018342_2030 (Interval in Earth days: 813) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.63 | 71.3 | 0.11 | 15.86 | 41.5 | 43.9 |
| Mawrth Vallis Phyllosilicates: PSP_007019_1980 ESP_077041_1980 (Interval in Earth days: 5456) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.68 | 336. | 0.65 | 16.95 | 38.6 | 38.7 |
| 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 |
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