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.
| Fluvial Erosion and Resistant Layering along Canyon Wall: ESP_027552_1735 ESP_027275_1735 (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 | -6.54 | 274. | -0.8 | 18.50 | 57.0 | 55.9 |
| Field of Shallow Depressions: ESP_027581_2185 ESP_028504_2185 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.22 | 197. | -3.7 | 29.11 | 45.6 | 52.4 |
| Candidate Future Landing Site in Elysium Planitia: ESP_027702_1815 ESP_026792_1815 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.616 | 138. | -0.1 | 20.11 | 52.8 | 50.8 |
| Light-Toned Rock Exposure in Crater Wall: ESP_027576_1560 ESP_028275_1560 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.6 | 341. | 3.03 | -10.8 | 66.9 | 64.2 |
| Fractured Source Region of Kasei Valles: ESP_027406_2020 ESP_027261_2020 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.79 | 295. | 4.55 | -14.6 | 45.0 | 46.1 |
| Unconformity in North Polar Layered Deposits: ESP_027679_2600 ESP_027798_2600 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.98 | 22.2 | 5.09 | -9.31 | 62.2 | 64.4 |
| Crater on Northern Plains: ESP_027768_2525 ESP_027860_2525 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 72.44 | 126. | -9.8 | 16.98 | 59.9 | 59.0 |
| Coloe Fossae: ESP_027507_2190 ESP_027573_2190 (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 | 39.24 | 55.4 | 11.1 | -3.33 | 43.9 | 45.6 |
| North Polar Dunes Change Detection: ESP_027581_2615 ESP_027396_2615 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.31 | 182. | -6.6 | 8.148 | 62.7 | 60.2 |
| Flow Lobes Resting on the Elevated Platform of a Moated Crater: ESP_027708_1815 ESP_027985_1815 (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 | 1.526 | 334. | 6.95 | -8.68 | 52.4 | 53.7 |
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