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.
| Flow Feature on Eos Chasma Wall: PSP_007389_1665 ESP_026324_1665 (Interval in Earth days: 1475) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.4 | 317. | -2.5 | 19.41 | 51.1 | 59.2 |
| Distal Rampart of Crater in Isidis Region: PSP_007740_1920 ESP_016047_1920 (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 | 12.01 | 89.5 | -2.3 | 18.67 | 43.2 | 38.0 |
| Fresh Double-Layered Ejecta Crater: PSP_007947_2350 PSP_009160_2350 (Interval in Earth days: 95) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.48 | 190. | 0.23 | -18.0 | 46.6 | 47.1 |
| Dark Dunes Over Light-Toned Mega-Ripples Seen in MOC Image SP1-26004: PSP_007532_1905 PSP_008679_1905 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.61 | 9.06 | 2.36 | -9.87 | 41.8 | 49.2 |
| Northern Plains with Mounds and Filled Crater: PSP_007738_2480 PSP_007804_2480 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.79 | 132. | 4.04 | -4.67 | 54.6 | 54.7 |
| Bacolor Crater Interior and Central Peak: PSP_007106_2135 PSP_009677_2135 (Interval in Earth days: 200) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.99 | 118. | 0.49 | -21.5 | 41.8 | 47.5 |
| 3-Kilometer Diameter Crater with Good Bedrock Exposures in Upper Walls: PSP_007892_1865 ESP_079800_1865 (Interval in Earth days: 5603) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.625 | 259. | 4.25 | -7.35 | 45.6 | 54.0 |
| 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 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 |
| Ridges and Mounds Near Hecates Tholus: PSP_007672_2155 PSP_007883_2155 (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 | 34.92 | 142. | 6.64 | -7.98 | 40.8 | 42.0 |
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