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.
Cones at Edge of North Polar Layered Deposits: ESP_018295_2580 ESP_026985_2580 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.99 | 263. | -6.6 | -21.3 | 57.3 | 57.6 |
Channel and Depression in Northeast Syrtis Major Planum: ESP_018210_1980 ESP_034772_1980 (Interval in Earth days: 1290) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.69 | 76.8 | 4.91 | -22.5 | 45.9 | 45.4 |
Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae: ESP_018225_2275 ESP_018146_2275 (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 | 47.18 | 22.7 | 5.82 | -17.3 | 43.5 | 45.3 |
Bull's-Eye Impact Crater: ESP_018522_2270 ESP_019010_2270 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.56 | 194. | 2.26 | -21.5 | 45.4 | 51.7 |
Future Mars Landing Site in Acidalia Mensa: ESP_018161_2270 ESP_018227_2270 (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 | 46.68 | 331. | -1.6 | -15.5 | 43.8 | 45.4 |
Future Mars Landing Site in Antoniadi Crater: ESP_018105_2045 ESP_018250_2045 (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 | 24.05 | 63.0 | -0.2 | 13.32 | 44.2 | 43.5 |
North Polar Residual Cap: ESP_017999_2720 ESP_018224_2720 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.01 | 275. | -19. | -13.0 | 65.6 | 65.5 |
Bedrock Exposures on Crater Floor in Terra Sabaea-Tyrhenna Terra Boundary: ESP_017815_1575 ESP_018527_1575 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.0 | 66.6 | -3.7 | 12.19 | 68.4 | 66.9 |
Light-Toned Outcrops in Noctis Labyrinthus: ESP_017768_1720 ESP_025271_1720 (Interval in Earth days: 585) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.75 | 267. | -3.0 | -29.2 | 58.6 | 51.1 |
Mounds and Polygonal Features in Crater: ESP_018078_2445 ESP_018210_2445 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 64.31 | 70.3 | 10.5 | -7.11 | 48.1 | 50.0 |
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