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.
Marte Vallis Streamlined Landforms: ESP_014092_1955 ESP_014158_1955 (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 | 15.46 | 183. | -6.8 | -25.9 | 48.1 | 48.6 |
Gully-Like Features on Dunes in MOC Image R10-03153: ESP_014067_1150 ESP_021583_1150 (Interval in Earth days: 586) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -64.5 | 158. | -5.6 | 20.41 | 53.4 | 51.9 |
Possible Rootless Cones in Hydraotes Chaos: ESP_013177_1800 ESP_021458_1800 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.053 | 326. | -4.9 | -21.2 | 49.8 | 53.9 |
Geologic Contact North of Arabia Terra: ESP_014138_2235 ESP_022643_2235 (Interval in Earth days: 662) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.14 | 3.39 | -2.8 | 24.50 | 67.8 | 69.9 |
Central Structure of a Large Impact Crater: ESP_013134_1610 ESP_021494_1610 (Interval in Earth days: 652) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.6 | 62.6 | -6.3 | 14.94 | 43.1 | 44.9 |
Fretted Terrain-Like Aprons Near Reull Vallis: ESP_012935_1415 ESP_013212_1415 (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 | -38.2 | 96.9 | 6.90 | -17.4 | 43.4 | 41.9 |
Channels and Noachian Crater Fill: ESP_012709_1445 ESP_013197_1445 (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 | -35.2 | 146. | 1.58 | -27.4 | 46.6 | 42.6 |
Channel Carved Into Scarp within Isidis Planitia: ESP_013186_1945 ESP_013252_1945 (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 | 14.55 | 78.4 | -2.7 | -24.1 | 58.1 | 58.9 |
Impact Crater with a Rocky Central Uplift: ESP_012947_1735 ESP_022441_1735 (Interval in Earth days: 740) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.55 | 125. | 4.88 | 27.14 | 48.6 | 37.0 |
Faulting in South Polar Layered Deposits: ESP_012762_1070 ESP_013171_1070 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -72.9 | 146. | 10.3 | -12.8 | 58.0 | 56.3 |
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