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.
| Gully Monitoring : ESP_049035_1395 ESP_049180_1395 (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 | -40.2 | 217. | -5.1 | 9.161 | 35.1 | 34.4 |
| Steep-Front Deposit on Crater Floor in Northern Arabia Terra: ESP_049293_2140 ESP_049359_2140 (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 | 33.61 | 3.59 | -1.5 | -17.5 | 60.0 | 59.9 |
| South Polar Layered Deposits: ESP_049272_0920 ESP_049060_0920 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.8 | 266. | 18.0 | 28.85 | 69.7 | 66.4 |
| Fan in Eastern Candor Chasma : ESP_049098_1730 ESP_057142_1730 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.80 | 292. | -0.6 | -15.4 | 35.0 | 44.8 |
| Constriction in Western Arm of Athabasca Valles Flood Lava : ESP_049143_1840 ESP_049499_1840 (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 | 4.002 | 141. | 4.44 | 20.81 | 39.9 | 34.9 |
| Rifts and Pitted Cones in Utopia Planitia : ESP_049039_2110 ESP_057782_2110 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.70 | 97.8 | 1.95 | 11.30 | 60.7 | 61.2 |
| Small Crater with Gullies: ESP_049261_1455 ESP_049828_1455 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.2 | 165. | 0 | 21.19 | 32.8 | 35.9 |
| Candidate Landing Site for 2020 Mission in Eberswalde Crater : ESP_049110_1560 ESP_049176_1560 (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 | -23.7 | 326. | 1.29 | -19.5 | 30.9 | 32.3 |
| Well-Preserved 3-Kilometer Impact Crater : ESP_049070_1940 ESP_058947_1940 (Interval in Earth days: 769) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.93 | 334. | -3.3 | 6.46 | 47.8 | 35.7 |
| Circular Structure in Lava in Southwestern Elysium Planitia : ESP_049011_1815 ESP_050145_1815 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.458 | 146. | 2.83 | 26.32 | 40.0 | 29.7 |
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