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.
| Channels near Osuga Valles: ESP_089041_1635 ESP_089463_1635 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.2 | 319. | 29.7 | 15.43 | 63.4 | 63.3 |
| Chryse Chaos: ESP_089120_1850 ESP_089265_1850 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.033 | 322. | 3.73 | 17.70 | 53.5 | 52.6 |
| Kasei Valles Alluvial Fans and Terraced Scarps: ESP_089042_2025 ESP_088765_2025 (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 | 22.38 | 291. | -8.7 | 22.53 | 48.3 | 44.7 |
| Test for Inverted Channel near Intersection with Crater: ESP_088921_1875 ESP_089066_1875 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.249 | 356. | -5.0 | 8.307 | 53.0 | 52.2 |
| Terrain Features around Crater in Arabia Terra: ESP_088875_2215 ESP_088585_2215 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.06 | 167. | 2.85 | -12.9 | 44.9 | 45.1 |
| Gypsum Dunes and Basal Unit Contact: ESP_089030_2605 ESP_088911_2605 (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 | 80.49 | 242. | -7.7 | 7.217 | 60.3 | 58.6 |
| Alluvial Fan and Light-Toned Deposits in Coprates Catena Trough: ESP_089187_1655 ESP_089121_1655 (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 | -14.1 | 297. | -21. | 2.298 | 65.3 | 63.9 |
| Depression in Nepenthes Mensae: ESP_088956_1935 ESP_089167_1935 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.27 | 119. | 1.73 | -7.93 | 50.0 | 51.2 |
| Ismenius Cavus Channel: ESP_088986_2140 ESP_089131_2140 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.50 | 17.7 | 2.34 | 12.95 | 45.5 | 45.3 |
| Flow Entering Fretted Terrain Valley: ESP_089025_2170 ESP_089091_2170 (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 | 36.42 | 31.9 | 6.73 | -11.0 | 45.2 | 47.2 |
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