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.
| 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 |
| Reull Vallis: PSP_007819_1390 PSP_009612_1390 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.6 | 99.6 | -6.4 | 7.67 | 74.7 | 81.0 |
| Possible Submarine Fan in Eastern Portion of Small Melas Chasma Basin: PSP_007377_1700 PSP_008379_1700 (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 | -9.82 | 283. | 5.56 | -6.99 | 48.4 | 58.5 |
| Complex Layered Deposits in Tithonium Chasma: PSP_007918_1755 PSP_008274_1755 (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 | -4.64 | 270. | 6.16 | -5.59 | 51.1 | 54.6 |
| Well-Exposed Central Uplift in Unnamed Crater: PSP_007109_1555 ESP_019385_1555 (Interval in Earth days: 956) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.2 | 43.4 | 7.44 | -4.41 | 53.1 | 65.2 |
| Fine-Branched Ridges: PSP_007474_1745 ESP_024497_1745 (Interval in Earth days: 1327) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.38 | 154. | 4.28 | 27.74 | 47.3 | 36.8 |
| Polygonal Fractures in Utopia Planitia: PSP_008069_2195 PSP_008504_2195 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.95 | 102. | -5.9 | 5.466 | 42.2 | 41.3 |
| Hematite in West Candor Chasma: PSP_007601_1745 PSP_010449_1745 (Interval in Earth days: 222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.55 | 286. | 7.08 | -20.0 | 48.5 | 59.7 |
| 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 |
| 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 |
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