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.
| 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 |
| Diverse Lava Morphologies in Elysium Planitia: ESP_017271_1870 ESP_017416_1870 (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 | 6.820 | 155. | -6.6 | 7.712 | 48.9 | 48.5 |
| Western Half of Well-Preserved 13-Kilometer Impact Crater: ESP_017067_2240 ESP_016144_2240 (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 | 43.44 | 319. | 5.46 | -4.73 | 41.5 | 45.2 |
| 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 |
| Valleys on Southern Flank of Apollinaris Patera: ESP_017099_1680 ESP_017244_1680 (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 | -11.6 | 174. | -11. | 3.166 | 58.8 | 58.8 |
| Putative Chlorides near Columbus Crater: ESP_017283_1490 ESP_017428_1490 (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 | -30.5 | 193. | -13. | -0.28 | 73.1 | 73.1 |
| 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 |
| Candidate MSL Landing Site in Northeast Syrtis Major: ESP_016931_1980 ESP_017076_1980 (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 | 17.80 | 77.0 | -4.2 | 8.612 | 43.0 | 42.6 |
| Fluvial Features Northwest of the Elysium Region: ESP_017285_2140 ESP_017707_2140 (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 | 33.83 | 128. | 5.01 | -9.66 | 40.6 | 42.5 |
| 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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