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.
| Cross-Section Through a Long Alba Patera Lava Flow Provided by a Graben: ESP_017162_2175 ESP_017228_2175 (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 | 37.20 | 246. | 7.11 | -11.0 | 40.4 | 42.0 |
| Crater with Gullies in Acidalia Planitia: ESP_017080_2285 ESP_017502_2285 (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 | 47.90 | 323. | 4.87 | -6.70 | 42.6 | 43.2 |
| Strike Slip Faults in Amazonis Planitia: ESP_017045_2015 ESP_018113_2015 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.26 | 204. | -6.1 | 8.022 | 42.8 | 44.3 |
| Rocky Hill: ESP_016922_1615 ESP_017423_1615 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.5 | 326. | 5.41 | 22.56 | 61.0 | 63.1 |
| Bedrock Exposures in Northwest Coprates Chasma: ESP_016976_1705 ESP_017187_1705 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.54 | 290. | 10.2 | -0.26 | 55.3 | 57.3 |
| Well-Preserved Mid-Latitude Crater: ESP_016981_2210 ESP_017482_2210 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.75 | 149. | -6.3 | 6.555 | 42.1 | 40.9 |
| Light-Toned Mounds in Acidalia Planitia: ESP_017132_2250 ESP_017633_2250 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.43 | 345. | -6.6 | 5.659 | 42.7 | 41.6 |
| Angular Unconformity in Cerberus Fossae Wall: ESP_017218_1890 ESP_017719_1890 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.971 | 162. | -10. | 8.2 | 48.0 | 48.3 |
| Enigmatic Pits in Southern Elysium Planitia: ESP_017284_1790 ESP_017429_1790 (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 | -1.07 | 160. | 5.24 | 19.21 | 52.3 | 52.0 |
| Coprates Chasma Wall: ESP_017200_1680 ESP_017912_1680 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.7 | 296. | -9.0 | 1.653 | 59.3 | 61.1 |
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