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 Pit and Chaos of A Lage Impact Crater: PSP_006908_1470 ESP_020173_1470 (Interval in Earth days: 1034) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.9 | 132. | 8.41 | -10.6 | 55.6 | 62.9 |
Basal Exposure of South Polar Layered Deposits: PSP_005102_1030 PSP_005155_1030 (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 | -76.8 | 132. | 7.05 | -13.4 | 60.2 | 62.0 |
Potentially Very Recent Impact Markings: PSP_005693_1650 ESP_011468_1650 (Interval in Earth days: 450) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.6 | 184. | 1.26 | 15.00 | 32.9 | 57.3 |
Light-Toned Layered Rock Outcrop in Ladon Vallis: PSP_006637_1590 ESP_023383_1590 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.8 | 330. | 7.10 | 20.68 | 44.1 | 31.2 |
Gratteri Crater Continuous Ejecta Blanket: PSP_005521_1620 ESP_012786_1620 (Interval in Earth days: 566) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.6 | 200. | 3.46 | 27.99 | 32.5 | 44.9 |
Sinuous Ridges Among Yardangs in Aeolis Region: PSP_006894_1740 ESP_016058_1740 (Interval in Earth days: 714) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.87 | 151. | 3.67 | 17.05 | 41.0 | 43.8 |
Fresh 6-Kilometer Diameter Crater with Gullied Slopes: PSP_006663_1425 ESP_011436_1425 (Interval in Earth days: 372) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 343. | -1.7 | -15.2 | 55.0 | 65.7 |
Central Peak of Crater near Herschel Crater: PSP_006974_1635 PSP_007185_1635 (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 | -16.3 | 128. | 7.10 | -5.68 | 46.5 | 50.3 |
Light-Toned Layering along Plains Southwest of Melas Chasma: PSP_005584_1700 PSP_005729_1700 (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 | -9.91 | 279. | 4.99 | 21.16 | 32.8 | 31.4 |
Bright Layers in Hale Crater Ejecta: PSP_006756_1465 ESP_023779_1465 (Interval in Earth days: 1327) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.2 | 322. | 4.57 | -11.2 | 53.6 | 43.7 |
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