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.
| Breached Impact Crater in Elysium Planitia: PSP_004151_1810 ESP_020963_1810 (Interval in Earth days: 1310) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.869 | 160. | 1.37 | -21.1 | 50.9 | 56.5 |
| Gullies in Southern Latitude Crater: PSP_004145_1455 ESP_013098_1455 (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 | -34.3 | 329. | -0.1 | -21.4 | 42.1 | 43.2 |
| Gullies in Small Crater within Kaiser Crater: PSP_003418_1335 PSP_003708_1335 (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 | -46.0 | 18.8 | 1.32 | 23.79 | 54.6 | 48.4 |
| Lobate Deposit and Mesa Near Reull Vallis: PSP_003217_1355 ESP_046890_1355 (Interval in Earth days: 3403) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.3 | 105. | 7.75 | -8.47 | 56.9 | 61.5 |
| Gullies in the North-Facing Wall of a Crater: PSP_003215_1405 PSP_003492_1405 (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 | -38.9 | 160. | -6.5 | -26.6 | 56.4 | 54.0 |
| Dark Materials on Block in Olympus Mons Aureole: PSP_003806_1975 ESP_012627_1975 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.32 | 217. | 2.81 | 19.24 | 61.8 | 61.8 |
| Light-Toned Outcrops in the Plains Between Melas and Candor Chasma: PSP_004318_1730 PSP_004740_1730 (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 | -6.84 | 282. | -3.1 | -15.3 | 45.8 | 41.7 |
| Mangala Valles Cataract: PSP_003991_1645 PSP_004347_1645 (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 | -15.3 | 210. | 0 | 10.73 | 46.2 | 41.2 |
| Unnamed Well-Preserved Crater within the Isidis Basin: PSP_003560_1900 PSP_005828_1900 (Interval in Earth days: 177) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.16 | 94.5 | 0.61 | 10.89 | 58.6 | 37.6 |
| Odd Layered and Eroding Crater Fill in Deeply Eroded Craters: PSP_003773_1630 PSP_003918_1630 (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 | -16.8 | 42.7 | 1.82 | 18.06 | 48.1 | 45.3 |
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