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.
Exposed Strata Near Melas Region Wall: ESP_013719_1665 ESP_021789_1665 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 289. | 2.48 | -8.89 | 37.2 | 44.6 |
Bright Gully Deposits in Western Hale Crater: ESP_013230_1445 ESP_014074_1445 (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 | -35.0 | 322. | 8.51 | -20.1 | 39.3 | 37.8 |
Edge of Fluidized Ejecta Rampart with Great Phyllosilicate Signature: ESP_012909_1680 ESP_013331_1680 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.9 | 83.6 | 3.17 | -12.0 | 47.1 | 43.1 |
Inverted Terrain in the Mawrth Vallis Region: ESP_013084_2060 ESP_013361_2060 (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 | 25.90 | 341. | 0.94 | -25.7 | 66.4 | 65.7 |
Gullies in Gorgonum Chaos Mesas: ESP_012747_1425 ESP_013024_1425 (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 | -37.0 | 189. | 2.86 | -20.5 | 46.1 | 44.2 |
Well-Preserved Gullied Impact Crater: ESP_013962_1430 ESP_021676_1430 (Interval in Earth days: 601) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.7 | 138. | 0.22 | -12.7 | 36.6 | 43.8 |
Gullies and Light-Toned Layers in Crater Walls in Terra Cimmeria: ESP_013328_1410 ESP_014185_1410 (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 | -38.6 | 168. | -6.9 | 18.35 | 39.9 | 37.0 |
Ejecta Flow from Bacolor Crater: ESP_014147_2135 ESP_022494_2135 (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 | 33.32 | 118. | -1.3 | -27.5 | 59.9 | 66.5 |
Bedrock Exposures in Uzboi Vallis and a Crater Rim: ESP_013586_1490 ESP_021722_1490 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.8 | 323. | -0.0 | -28.7 | 36.4 | 44.3 |
10 Kilometer Diameter Rayed Crater: ESP_012738_1785 ESP_013094_1785 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.41 | 70.8 | 2.49 | 14.97 | 53.0 | 48.7 |
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