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 Well-Preserved Crater: ESP_013198_1660 ESP_021545_1660 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 113. | 8.48 | -27.9 | 42.6 | 48.8 |
Valley in Elysium Region Volcanic Rise: ESP_013157_2015 ESP_013658_2015 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.49 | 149. | -6.4 | 14.55 | 63.2 | 56.7 |
Steep Shields in Tharsis Region: ESP_014037_1760 ESP_014182_1760 (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 | -3.90 | 246. | -1.4 | 16.04 | 37.7 | 35.2 |
Incipient Scalloped Terrain in Mid-Latitude Mantle at Peneus Patera: ESP_013029_1235 ESP_013306_1235 (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 | -56.1 | 54.6 | -0.3 | -19.2 | 47.7 | 46.9 |
Tongue-Shaped Features within Alcoves on South Mid-Latitude Crater Wall: ESP_014058_1450 ESP_014335_1450 (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 | -34.5 | 37.1 | 1.29 | -21.3 | 36.0 | 39.2 |
Possible Sulfates in Ius Chasma: ESP_013759_1720 ESP_020550_1720 (Interval in Earth days: 529) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.88 | 276. | 4.68 | -17.6 | 38.5 | 55.9 |
Distal Ramparts for Fresh Crater Santa Fe in Chryse Planitia: ESP_012795_1995 ESP_013639_1995 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.03 | 312. | -0.8 | -24.0 | 63.6 | 57.4 |
Hydrated Minerals and Gully on Central Uplift of Li Fan Crater: ESP_013564_1330 ESP_013709_1330 (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 | -46.8 | 207. | -5.9 | 5.732 | 40.8 | 39.9 |
A Fan in a Southern Highlands Crater: ESP_014159_1670 ESP_020106_1670 (Interval in Earth days: 464) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 157. | -7.0 | 7.119 | 34.6 | 56.0 |
Gullies on Southwest Slope of Asimov Crater: ESP_012767_1320 ESP_012912_1320 (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 | -47.5 | 4.40 | 10.5 | 21.65 | 47.2 | 44.3 |
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