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.
| Xanthe Dorsa: ESP_066965_2140 ESP_067176_2140 (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 | 33.69 | 331. | -5.3 | 17.45 | 63.6 | 59.5 |
| Chryse Chaos: ESP_067005_1940 ESP_066794_1940 (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 | 13.96 | 321. | 2.33 | -22.6 | 49.3 | 53.3 |
| Scarp in East Candor Chasma: ESP_067059_1735 ESP_066927_1735 (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 | -6.39 | 291. | -6.2 | 17.46 | 40.1 | 39.1 |
| Steep Rocky Slopes in Central Valles Marineris: ESP_067257_1665 ESP_066439_1665 (Interval in Earth days: 64) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.1 | 290. | -15. | 6.069 | 39.2 | 41.7 |
| Chaotic Terrain in Xanthe Terra: ESP_066913_1780 ESP_075011_1780 (Interval in Earth days: 631) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.09 | 315. | -8.7 | -22.8 | 42.7 | 49.2 |
| Vent and Channel East of Olympus Mons: ESP_067061_1990 ESP_067404_1990 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.89 | 232. | 5.92 | 17.21 | 51.5 | 47.2 |
| Auqakuh Vallis: ESP_067054_2125 ESP_084409_2125 (Interval in Earth days: 1352) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.38 | 61.9 | 5.60 | -11.2 | 60.8 | 64.2 |
| Fans and Polygons: ESP_067026_0925 ESP_066959_0925 (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 | -87.2 | 167. | 8.81 | 21.59 | 72.0 | 69.8 |
| Esker Candidates near Mamers Valles: ESP_067280_2165 ESP_067412_2165 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.20 | 14.6 | 6.74 | -7.75 | 60.6 | 59.8 |
| Rim of Nansen Crater: ESP_067141_1295 ESP_073907_1295 (Interval in Earth days: 527) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -50.1 | 220. | -4.1 | 18.87 | 47.9 | 56.7 |
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