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.
| Bouldery Layered Slopes in Noctis Labyrinthus: ESP_027816_1725 ESP_028515_1725 (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 | -7.18 | 267. | 6.39 | -10.2 | 56.4 | 56.5 |
| Variable Relief of North Polar Layered Deposits: ESP_028182_2650 ESP_028010_2650 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.84 | 323. | -3.7 | 8.258 | 72.2 | 69.4 |
| Crater Central Uplift in Solis Planum: ESP_027987_1565 ESP_036914_1565 (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 | -23.2 | 281. | 9.65 | -2.23 | 64.3 | 66.0 |
| Cratered Cones within a Flow Unit in Grjota Valles: ESP_027978_1955 ESP_028466_1955 (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 | 15.18 | 162. | 6.83 | -12.0 | 48.6 | 52.8 |
| Small Shield in Tharsis Region Embayed by Younger Lavas: ESP_027988_2010 ESP_033658_2010 (Interval in Earth days: 442) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.48 | 248. | 5.19 | -6.24 | 47.9 | 39.0 |
| Crater on Lobate Apron: ESP_028083_2310 ESP_028162_2310 (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 | 50.88 | 175. | -23. | -2.19 | 55.5 | 54.6 |
| Scoured Crater Floor Adjacent to Fan-Shaped Form: ESP_028037_2140 ESP_033918_2140 (Interval in Earth days: 458) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.48 | 349. | 0.97 | -13.3 | 48.7 | 41.7 |
| Central Uplift of Crater in Lunae Planum: ESP_028092_1975 ESP_037309_1975 (Interval in Earth days: 718) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.38 | 291. | -7.8 | 6.232 | 50.0 | 53.4 |
| Fan in Crater West of Gale Crater: ESP_027900_1745 ESP_045570_1745 (Interval in Earth days: 1377) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.45 | 136. | -16. | 14.60 | 57.1 | 51.7 |
| Possible Noachian Phyllosilicate with Low-Ca Pyroxene Near Nili Fossae: ESP_027955_2020 ESP_028311_2020 (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 | 21.63 | 70.4 | -4.7 | 13.27 | 48.4 | 49.4 |
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