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.
| Faulted Plains in Tempe Terra: ESP_027842_2250 ESP_028198_2250 (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 | 44.42 | 272. | -6.0 | 8.621 | 49.1 | 52.1 |
| Arabia Terra Sample: ESP_027971_1905 ESP_030239_1905 (Interval in Earth days: 176) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.17 | 354. | -0.9 | 10.96 | 50.3 | 56.5 |
| Layered Bedrock on Crater Floor: ESP_028074_1605 ESP_028918_1605 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.4 | 66.2 | 4.51 | -9.37 | 62.1 | 58.5 |
| 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 |
| 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 |
| Fractures in Chryse Planitia: ESP_027959_1990 ESP_028737_1990 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.71 | 321. | -5.3 | 7.285 | 48.9 | 53.3 |
| Possible Future Landing Site in Mawrth Vallis: ESP_028011_2055 ESP_028288_2055 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.33 | 339. | 11.0 | -7.26 | 47.3 | 51.1 |
| 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 |
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