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.
| Mesa in Olympica Fossae: ESP_034146_2050 ESP_034436_2050 (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 | 24.78 | 246. | -8.3 | 18.70 | 40.6 | 39.1 |
| Pits and Channels on East Flank of Ascraeus Mons: ESP_034317_1955 ESP_034528_1955 (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 | 15.15 | 257. | 8.85 | -5.48 | 41.4 | 43.6 |
| Well-Preserved 4-Kilometer Impact Crater: ESP_034248_2175 ESP_034314_2175 (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 | 37.33 | 338. | 2.63 | -13.1 | 40.8 | 42.2 |
| Outflow Channel Features Associated with Small Chaotic Terrain: ESP_034355_1770 ESP_034922_1770 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.88 | 302. | 6.96 | -7.21 | 49.3 | 54.3 |
| Filled Crater Near Athabasca Valles: ESP_034123_1825 ESP_052571_1825 (Interval in Earth days: 1437) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.424 | 155. | 3.78 | -28.6 | 44.9 | 50.6 |
| Northern Plains Features: ESP_034200_2335 ESP_034266_2335 (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 | 53.02 | 205. | 4.92 | -6.54 | 46.1 | 46.6 |
| Small Cratered Cones and Strange Lava Flows South of Ascraeus Mons: ESP_034172_1880 ESP_035596_1880 (Interval in Earth days: 111) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.690 | 258. | -6.3 | 14.20 | 44.0 | 49.5 |
| Dark-Toned Pitted Mound in Crater in Northeast Arabia Terra: ESP_034324_2040 ESP_034970_2040 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.82 | 68.1 | -21. | -1.99 | 42.4 | 42.7 |
| Valleys and Fan Feature at Valley Terminus in Crater: ESP_034326_2000 ESP_035882_2000 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.63 | 11.6 | 4.33 | -16.3 | 40.8 | 47.8 |
| Meander in Central Channel in Nanedi Valles: ESP_034236_1855 ESP_035792_1855 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.183 | 310. | 3.71 | -19.7 | 44.7 | 53.6 |
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