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.
| Collapse Terrain Near Head of Ravi Vallis: ESP_050007_1780 ESP_059317_1780 (Interval in Earth days: 725) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.82 | 316. | 3.87 | -18.2 | 31.1 | 34.4 |
| Curved Ridge in Ismenius Lacus : ESP_049991_2245 ESP_049714_2245 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.01 | 27.9 | -2.2 | 10.03 | 58.6 | 62.0 |
| Pitted Material in Large Crater North of Hellas Planitia : ESP_049872_1580 ESP_050017_1580 (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 | -21.6 | 44.6 | 4.62 | 19.35 | 31.9 | 32.1 |
| Lava Channels in Daedalia Planum : ESP_049720_1595 ESP_049997_1595 (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 | -20.3 | 234. | -0.8 | -20.6 | 30.9 | 34.5 |
| Western Continuous Ejecta of Istok Crater in Thaumasia Fossae : ESP_049811_1345 ESP_049877_1345 (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 | -45.1 | 274. | -5.3 | -19.3 | 44.2 | 46.0 |
| Possible Pit at Edge of South Polar Residual Cap : ESP_049945_0930 ESP_049972_0930 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.1 | 263. | 7.78 | 0.683 | 80.0 | 81.4 |
| Darker Inverted Terrain Within Light-Toned Possibly Altered Terrain : ESP_049880_1410 ESP_049735_1410 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.8 | 188. | 6.06 | -14.4 | 40.3 | 39.7 |
| Intersection between Ejecta and Cone : ESP_050098_2205 ESP_050942_2205 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.19 | 345. | 7.36 | -26.0 | 53.6 | 46.5 |
| Alluvial Fans in Newton Crater : ESP_050051_1410 ESP_050130_1410 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.6 | 200. | -0.6 | 26.77 | 43.0 | 42.5 |
| Disrupted Terrain in Southern Elysium Planitia : ESP_049907_1770 ESP_058228_1770 (Interval in Earth days: 648) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.00 | 167. | -0.0 | 14.85 | 31.3 | 32.4 |
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