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.
| 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 |
| Central Uplift of an Impact Crater: ESP_017181_1735 ESP_024829_1735 (Interval in Earth days: 596) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.23 | 93.6 | 4.73 | -14.2 | 54.9 | 44.3 |
| Crater and Ejecta and Context for MOC Image SP2-47903: ESP_017046_2080 ESP_017824_2080 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.58 | 175. | 4.05 | -7.84 | 40.8 | 43.4 |
| 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 |
| 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 |
| Possible Phyllosilicate-Rich Terrain: ESP_016918_2030 ESP_017986_2030 (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 | 22.68 | 71.0 | -0.6 | 12.29 | 41.6 | 43.2 |
| East Rim of Well-Preserved Crater on Rim of Larger Crater: ESP_016971_1610 ESP_017683_1610 (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 | -18.5 | 69.1 | -0.5 | 8.387 | 61.8 | 65.0 |
| 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 |
| Possible Chlorites and Prehnite in Northern Plains Crater: ESP_016933_2310 ESP_017210_2310 (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 | 50.48 | 16.5 | 4.76 | -14.3 | 43.8 | 44.8 |
| 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 |
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