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.
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010808_2720 ESP_028150_2680 (Interval in Earth days: 1351) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.93 | 95.5 | -6.3 | -11.4 | 79.4 | 74.3 |
| Well-Preserved Impact Crater on Northern Plains: PSP_010559_2170 ESP_016005_2170 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.54 | 155. | 5.58 | -8.20 | 52.5 | 43.4 |
| Complex Morphology in Acidalia Region: ESP_011384_2185 ESP_011661_2185 (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 | 38.01 | 310. | 7.35 | -13.2 | 63.5 | 68.9 |
| Mesas with Circumferential Depressions Near Kasei Valles: ESP_011319_2100 ESP_011464_2100 (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 | 29.64 | 289. | -20. | -7.41 | 62.3 | 62.9 |
| Section of Wall Rock on the South Rim of Coprates Chasma: PSP_010501_1645 ESP_016026_1645 (Interval in Earth days: 431) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 305. | 5.32 | 23.12 | 62.0 | 48.0 |
| Central Uplift of an Impact Crater: PSP_010745_1465 ESP_028006_1465 (Interval in Earth days: 1345) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.2 | 126. | 5.23 | -17.2 | 69.4 | 71.8 |
| Light-Toned Layering South of Ius Chasma with Unusual Morphology: PSP_010423_1720 ESP_016726_1720 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.01 | 275. | -10. | 7.863 | 60.0 | 52.5 |
| Possible MSL Landing Site in Holden Crater: ESP_011397_1535 ESP_011898_1535 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.3 | 324. | 3.35 | 27.36 | 61.3 | 54.6 |
| Flow Feature in Southern Utopia Planitia: ESP_011497_1965 ESP_064454_1965 (Interval in Earth days: 4126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.22 | 110. | -4.3 | -24.5 | 59.6 | 61.7 |
| Crater Wall in Chryse Planitia: PSP_010408_2070 ESP_045906_2070 (Interval in Earth days: 2766) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.88 | 319. | 2.47 | -6.79 | 50.6 | 48.1 |
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