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.
| Gullies in Light-Toned Rock: ESP_012795_1395 ESP_013507_1395 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.2 | 319. | 2.74 | 16.59 | 45.9 | 37.2 |
| Layering in Argyre Planitia Sinuous Ridge: ESP_012927_1245 ESP_013626_1245 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.1 | 318. | 1.77 | -23.3 | 48.2 | 46.0 |
| Exposure of Layers in South Gale Crater with Possible Sulfates: ESP_014186_1745 ESP_020410_1745 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.56 | 138. | 8.10 | -13.1 | 35.2 | 55.9 |
| Western Half of Very Well-Preserved Gullied Crater: ESP_012807_1505 ESP_012952_1505 (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 | -29.4 | 351. | -5.9 | 9.919 | 45.8 | 42.6 |
| Valley with Central Ridge Located North of Schiaparelli Crater: ESP_014164_1870 ESP_020388_1870 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.827 | 16.4 | 19.0 | -0.77 | 40.3 | 55.8 |
| Hill and Adjacent Depression in Polar Layered Deposits: ESP_012815_1080 ESP_013013_1080 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.7 | 141. | 1.59 | -20.3 | 57.3 | 57.1 |
| Stratigraphic Relations in THEMIS Image V11134006 in Sinus Meridiani: ESP_013703_1800 ESP_021984_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 | -0.14 | 2.99 | 25.0 | 10.04 | 41.4 | 46.9 |
| Ares Vallis Wall and Floor Exposures: ESP_013216_1870 ESP_022143_1870 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.694 | 340. | -2.5 | 20.39 | 53.0 | 48.5 |
| Ejecta Falling Into Earlier Large Crater: ESP_013346_1940 ESP_013768_1940 (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 | 13.86 | 29.4 | 6.71 | -7.95 | 55.5 | 51.3 |
| Chain of Cones and Craters in Isidis Planitia: ESP_013054_1900 ESP_013199_1900 (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 | 9.766 | 83.1 | -5.1 | 9.582 | 56.5 | 54.2 |
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