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.
| Mesas in Huo Hsing Vallis: PSP_007688_2075 PSP_008690_2075 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.10 | 66.7 | 5.61 | -11.4 | 40.1 | 43.9 |
| Potential Fan Deposit in Ritchey Crater with Clays: PSP_007363_1510 PSP_008365_1510 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.4 | 308. | 3.89 | -7.30 | 59.7 | 71.0 |
| 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 |
| Crater in the Adamas Labyrinthus Region Seen in THEMIS Image V21701005: PSP_007713_2170 PSP_009862_2170 (Interval in Earth days: 167) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.45 | 103. | -4.4 | 10.64 | 41.9 | 45.6 |
| Southern Branch of Kasei Valles: PSP_007891_1980 ESP_036162_1980 (Interval in Earth days: 2203) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.93 | 285. | -6.1 | 8.571 | 42.8 | 47.1 |
| 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 |
| 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 |
| Flow-Banded Deformed Terrain of Hellas Basin Floor: PSP_007201_1405 PSP_007491_1405 (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 | -38.9 | 54.9 | -7.0 | 3.906 | 65.3 | 68.9 |
| Upper Section of Northern Olympus Mons Basal Scarp: PSP_007445_2035 PSP_008447_2035 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 223. | -1.4 | -13.8 | 40.1 | 44.4 |
| Geologic Contacts in Mangala Valles: PSP_007617_1750 PSP_007973_1750 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.85 | 209. | 5.90 | -6.28 | 48.4 | 52.6 |
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