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.
| Acidalia Planitia: PSP_007415_2300 PSP_008140_2300 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.44 | 319. | -3.8 | 17.50 | 47.5 | 42.5 |
| Layers in Arnus Vallis: PSP_007187_1925 PSP_010404_1925 (Interval in Earth days: 251) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.51 | 69.9 | -2.9 | 14.53 | 39.6 | 51.3 |
| Area Near Summit of Gale Crater Mound: PSP_008002_1750 PSP_009927_1750 (Interval in Earth days: 151) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.85 | 137. | -5.8 | -22.8 | 52.8 | 59.9 |
| Central Peak of Fesenkov Crater: PSP_007931_2020 ESP_024585_2020 (Interval in Earth days: 1298) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.68 | 273. | -8.3 | -25.5 | 42.4 | 39.6 |
| Putative Salt Deposits Detected by THEMIS West of Meridiani Region: PSP_007770_1770 PSP_008917_1770 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.17 | 351. | 6.87 | -11.5 | 49.0 | 57.2 |
| Hellas Planitia: PSP_007913_1370 ESP_016642_1370 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.6 | 52.4 | 1.81 | 18.41 | 76.8 | 74.9 |
| Very Recent Small Crater in Dejnev Crater: PSP_008145_1545 ESP_027067_1545 (Interval in Earth days: 1474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.0 | 195. | -8.7 | 6.238 | 66.9 | 69.0 |
| Inner Channel Deposit in Kasei Vallis: PSP_007825_2010 ESP_035463_2010 (Interval in Earth days: 2153) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.84 | 287. | -3.9 | 12.13 | 41.7 | 43.8 |
| Cut Crater in Ganges Chasma: PSP_008101_1710 ESP_016263_1710 (Interval in Earth days: 636) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.91 | 314. | -5.3 | 21.95 | 55.9 | 47.3 |
| Knobs and Cones in Acidalia Planitia: PSP_007506_2220 ESP_051759_2220 (Interval in Earth days: 3448) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.57 | 354. | 3.16 | 20.33 | 43.2 | 38.9 |
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