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.
| Fading Rayed Crater in Daedalum Planum: PSP_007735_1570 ESP_028345_1570 (Interval in Earth days: 1606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 230. | 2.03 | -10.9 | 60.9 | 63.5 |
| Mounds in Cydonia Region: PSP_007770_2205 PSP_007981_2205 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.03 | 345. | 7.20 | -6.26 | 41.7 | 42.5 |
| Faulted Layered Deposits in Eastern Candor Chasma: PSP_007192_1710 PSP_008049_1710 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.72 | 295. | 7.77 | -11.1 | 45.4 | 55.7 |
| Central Peak of Large 40-Kilometer Diameter Crater: PSP_007592_1995 ESP_045595_1995 (Interval in Earth days: 2961) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.25 | 169. | -0.9 | 19.06 | 40.8 | 43.5 |
| Light-Toned Outcrops in North Melas Chasma Wall with Possible Sulfates: PSP_007390_1700 PSP_007680_1700 (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 | -9.78 | 289. | -8.0 | 6.442 | 49.4 | 51.7 |
| Landslide Scarp: PSP_007785_1645 PSP_008141_1645 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.1 | 303. | 7.47 | -3.79 | 56.0 | 60.0 |
| Pits at the Head of the Hephaestus Fossae: PSP_007264_1975 PSP_007554_1975 (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 | 17.42 | 127. | -7.3 | 5.253 | 40.1 | 40.3 |
| Geologic Contacts in Mangala Valles: PSP_007617_1750 PSP_007973_1750 (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 | -4.85 | 209. | 5.90 | -6.28 | 48.4 | 52.6 |
| 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 |
| Gullies Possibly Produced by Snow or Ice Melting: PSP_007270_2240 PSP_010487_2240 (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 | 43.42 | 319. | -2.8 | 11.76 | 45.5 | 52.4 |
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