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.
| Light-Toned Layering along Plains South of Ius Chasma: PSP_005149_1715 PSP_005215_1715 (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 | -8.36 | 275. | 4.52 | -19.5 | 35.5 | 36.7 |
| Cratered Cones Near Hephaestus Fossae: PSP_004060_2020 ESP_057069_2020 (Interval in Earth days: 4131) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.73 | 121. | 9.17 | -20.1 | 63.3 | 62.5 |
| South Polar Layered Deposits: PSP_005011_0885 PSP_005023_0915 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.4 | 191. | 16.5 | 16.24 | 69.4 | 68.8 |
| Geologic Contacts Near Ganges Chasma: PSP_005082_1700 ESP_011991_1700 (Interval in Earth days: 538) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.68 | 305. | -2.8 | 14.87 | 36.1 | 54.7 |
| Exposed Faults in Coprates Chasma Wall: PSP_005069_1670 PSP_005702_1670 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.8 | 299. | 3.35 | -20.7 | 34.9 | 34.6 |
| The Edge of Olympus Mons: PSP_005019_1970 PSP_005441_1970 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.02 | 221. | 2.77 | -13.5 | 51.3 | 46.9 |
| Small Scallops Suggesting Sublimation O North Bank of Auqakuh Vallis: PSP_003482_2115 PSP_005895_2115 (Interval in Earth days: 188) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.05 | 60.7 | 6.34 | 26.06 | 68.8 | 48.6 |
| Potential Currently-Active Gullies in Fresh Crater: PSP_003939_1420 ESP_012549_1420 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.6 | 192. | 7.82 | 27.83 | 44.6 | 47.0 |
| Intriguing Dark Dunes in Proctor Crater: PSP_003101_1320 ESP_011909_1320 (Interval in Earth days: 686) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.7 | 30.6 | 22.7 | -2.86 | 58.7 | 61.9 |
| Light Toned Ridges in Meridiani Region: PSP_003682_1805 PSP_003972_1805 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.329 | 5.15 | -0.2 | 29.79 | 54.2 | 50.0 |
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