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.
| Phlegra Montes: ESP_075346_2165 ESP_093055_2165 (Interval in Earth days: 1380) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.21 | 162. | 7.16 | -14.4 | 69.2 | 69.2 |
| Canyon Floor in East Coprates Chasma: ESP_075407_1650 ESP_075473_1650 (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 | -15.0 | 304. | -4.1 | -21.8 | 38.2 | 39.0 |
| Aram Chaos Mineralogical Variability: ESP_075432_1840 ESP_075788_1840 (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 | 3.921 | 339. | 1.37 | 17.51 | 45.8 | 40.6 |
| Channel and Crater North of Huygens Crater: ESP_075416_1745 ESP_075772_1745 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.39 | 57.5 | 0.14 | 18.63 | 41.3 | 36.4 |
| Small Delta or Fan: ESP_075437_1370 ESP_076426_1370 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.5 | 209. | -3.2 | 6.092 | 39.4 | 47.0 |
| Scarp Monitoring: ESP_075270_1190 ESP_075613_1190 (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 | -60.7 | 92.0 | -2.1 | -18.0 | 48.1 | 50.6 |
| Potential Amazonian Delta Deposit within Darwin Crater: ESP_075485_1230 ESP_075775_1230 (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 | -56.4 | 342. | -3.6 | 17.72 | 46.2 | 46.9 |
| Candidate Mud Volcano near Zhurong Rover Traverse: ESP_075348_2050 ESP_075414_2050 (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 | 24.79 | 109. | 0.08 | -16.3 | 60.9 | 61.0 |
| Possible Phyllosilicate-Rich Terrain in Crater near Her Desher Vallis: ESP_075354_1540 ESP_075921_1540 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.6 | 312. | 0.37 | 10.62 | 36.7 | 34.4 |
| Layers at Edge of Pedestal Crater in Tikhonravov Crater: ESP_075364_1940 ESP_076353_1940 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.64 | 35.2 | -7.3 | 2.427 | 53.3 | 41.6 |
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