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.
| Distinctive Small Rayed Crater in Terra Cimmeria: PSP_010863_1720 ESP_020133_1720 (Interval in Earth days: 723) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.92 | 142. | -1.8 | -20.3 | 58.8 | 57.3 |
| Well-Preserved Unnamed Crater in Acidalia Planitia: PSP_010579_2170 ESP_016104_2170 (Interval in Earth days: 431) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.66 | 329. | 4.65 | 19.26 | 52.8 | 40.8 |
| Crater Wall in Chryse Planitia: PSP_010408_2070 ESP_045906_2070 (Interval in Earth days: 2766) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.88 | 319. | 2.47 | -6.79 | 50.6 | 48.1 |
| Wallrock and Light-Toned Layering Geologic Contact in Coprates Chasma: ESP_011385_1695 ESP_011451_1695 (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 | -10.2 | 290. | -2.8 | -24.8 | 58.4 | 60.0 |
| Possible MSL Landing Site Mawrth Vallis: PSP_010816_2040 PSP_010882_2040 (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 | 23.95 | 340. | 3.22 | -17.0 | 54.1 | 56.5 |
| Possible Source for a Small Outburst along the Cerberus Fossae: PSP_010480_1910 ESP_053362_1910 (Interval in Earth days: 3341) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.70 | 155. | 7.33 | -7.40 | 52.6 | 47.0 |
| Central Region of an Impact Crater: PSP_010812_1665 ESP_027730_1665 (Interval in Earth days: 1319) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 94.9 | 0.22 | 14.92 | 60.5 | 59.2 |
| Gale Crater - Potential MSL Landing Site: PSP_010639_1755 PSP_010573_1755 (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 | -4.49 | 137. | -2.2 | 21.20 | 57.9 | 56.0 |
| Possible Inverted Meanders in Filled Channel West of Ladon Valles: ESP_011476_1600 ESP_014100_1600 (Interval in Earth days: 205) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.8 | 327. | -4.0 | 9.389 | 59.7 | 33.0 |
| Mounds on Kashira Crater Floor: ESP_011370_1525 ESP_029053_1525 (Interval in Earth days: 1378) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 341. | 8.46 | -10.0 | 61.4 | 59.8 |
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