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.
| Echus Chasma Layered Deposits: ESP_042624_1790 ESP_069316_1790 (Interval in Earth days: 2080) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.04 | 280. | -4.9 | -22.9 | 44.0 | 55.8 |
| South Wall of East Candor Chasma: ESP_042017_1715 ESP_042162_1715 (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 | -8.56 | 294. | -2.6 | 13.34 | 40.8 | 41.4 |
| Utopia Region Knobs: ESP_042552_2185 ESP_042842_2185 (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 | 38.19 | 80.7 | 3.32 | 21.97 | 42.4 | 39.4 |
| Dense Gullies in East Argyre Region: ESP_042372_1325 ESP_051378_1325 (Interval in Earth days: 701) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.0 | 327. | -5.8 | 25.72 | 69.4 | 69.3 |
| Landscape Evolution in Cydonia Mensae: ESP_042318_2210 ESP_042595_2210 (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 | 40.41 | 350. | -5.3 | -28.4 | 45.5 | 45.8 |
| Crevasse-Like Features Utopia Region: ESP_042104_2210 ESP_042183_2210 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.82 | 74.7 | -19. | 6.575 | 48.4 | 45.8 |
| Pit in Ulysses Fossae: ESP_042678_1935 ESP_042744_1935 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.34 | 244. | -1.7 | -24.0 | 39.9 | 42.1 |
| Expanded Secondary Craters in Arcadia Planitia: ESP_042376_2305 ESP_044222_2305 (Interval in Earth days: 144) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.36 | 203. | 3.58 | 19.36 | 49.6 | 40.0 |
| Acidalia Planitia Slope-Monitoring Site: ESP_042253_2185 ESP_043110_2185 (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 | 38.33 | 324. | -0.6 | 13.27 | 44.6 | 39.4 |
| Flow Features in Mamers Valles: ESP_042238_2170 ESP_090186_2170 (Interval in Earth days: 3736) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.61 | 15.5 | -7.5 | 14.13 | 44.5 | 55.3 |
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