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.
| Dunes Dubbed Kaltain : ESP_053377_2570 ESP_053324_2570 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.62 | 89.4 | 0.57 | 16.87 | 54.7 | 53.6 |
| Dark Materials on Olympus Mons: ESP_012548_1980 ESP_013049_1980 (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 | 17.55 | 216. | -2.9 | 20.20 | 63.7 | 59.8 |
| Exit Breach in Well-Preserved Crater: ESP_053169_2170 ESP_053459_2170 (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 | 36.70 | 20.6 | 5.45 | 24.02 | 39.3 | 38.5 |
| Possible Tuff Ring near Apollinaris Mons: ESP_052913_1725 ESP_053770_1725 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.34 | 176. | 2.69 | 22.08 | 55.4 | 54.7 |
| Dunes Dubbed Laguna : ESP_053000_2525 ESP_053013_2525 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 72.40 | 305. | 1.60 | 17.00 | 51.5 | 50.4 |
| Constriction in Kasei Valles : ESP_053067_2045 ESP_053133_2045 (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 | 24.48 | 287. | 5.25 | -15.8 | 40.5 | 42.4 |
| Flow Field West of Arsia Mons: ESP_053188_1710 ESP_053333_1710 (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 | -8.68 | 228. | -6.2 | 7.728 | 57.5 | 56.7 |
| Dunes Dubbed Pismo Beach : ESP_053092_2530 ESP_053079_2530 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 72.57 | 309. | 14.3 | -1.20 | 50.8 | 51.8 |
| Collapse Terrain South of Orson Welles Crater: ESP_053198_1780 ESP_071530_1780 (Interval in Earth days: 1428) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.84 | 313. | 13.5 | -2.31 | 51.9 | 58.1 |
| Sand Sheet Characterization near Meroe Patera: ESP_052851_1870 ESP_052996_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 | 7.135 | 67.6 | -2.0 | 10.35 | 47.2 | 46.7 |
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