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.
| Flows into the Isidis Basin: PSP_007727_1830 PSP_008808_1830 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.147 | 85.9 | -5.8 | 5.575 | 46.5 | 52.1 |
| 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 |
| Layering in East Coprates Chasma Wall: PSP_007864_1655 PSP_007508_1655 (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 | -14.1 | 307. | -8.1 | 4.599 | 57.2 | 52.4 |
| Light-Toned Rock Exposures: PSP_007101_1730 ESP_019311_1730 (Interval in Earth days: 952) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.99 | 260. | -7.9 | 3.361 | 44.7 | 56.7 |
| Central Peak and Pit of Large Impact Crater: PSP_007027_1570 ESP_023905_1570 (Interval in Earth days: 1315) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.9 | 122. | 4.75 | -19.6 | 51.3 | 40.6 |
| Partially-Buried Pre-Existing Crater: PSP_007524_1400 ESP_016108_1400 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 234. | -1.4 | -18.6 | 70.0 | 67.6 |
| Unusually Large Gullies on Equator-Facing Slope of Crater: PSP_007692_2235 PSP_008694_2235 (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 | 43.35 | 315. | 2.62 | -10.7 | 43.2 | 43.3 |
| Fine Layered Deposits in Capri Mensa: PSP_008088_1670 PSP_008378_1670 (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 | -12.8 | 310. | -6.2 | 5.9 | 58.3 | 59.7 |
| Big Fresh Crater with a Gullied Central Peak: PSP_007845_2190 PSP_008135_2190 (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 | 38.53 | 99.2 | -5.6 | 5.818 | 42.3 | 41.1 |
| Fresh Double Layer Ejecta Crater in Northern Plains: PSP_007736_2345 PSP_008303_2345 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.37 | 190. | 8.23 | -7.73 | 47.0 | 45.9 |
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