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.
| Lobate Flows in Phlegra Dorsa: ESP_065810_2130 ESP_075016_2130 (Interval in Earth days: 717) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.59 | 171. | -2.4 | 6.659 | 73.2 | 69.7 |
| Slope Failures in Tempe Terra: ESP_065925_2175 ESP_066057_2175 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.31 | 273. | -9.9 | -28.1 | 76.5 | 77.1 |
| Gullies in Promethei Terra Crater: ESP_065866_1360 ESP_066011_1360 (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 | -43.7 | 93.7 | -4.1 | 22.17 | 46.3 | 42.7 |
| Pit in Mid-Latitude Deposit: ESP_065905_1315 ESP_066591_1315 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.3 | 109. | 1.16 | -13.6 | 46.5 | 44.1 |
| Gullies and Crater Fill: ESP_065798_1430 ESP_066220_1430 (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 | -36.8 | 148. | -4.5 | 27.39 | 46.2 | 39.2 |
| Central Pit Crater with Possibly Active Slope Processes: ESP_065704_1480 ESP_065770_1480 (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 | -31.6 | 191. | 7.68 | -6.72 | 46.3 | 46.6 |
| Gullies in Southern Hemisphere Crater: ESP_065915_1410 ESP_066047_1410 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.8 | 195. | -7.9 | -28.7 | 45.3 | 45.6 |
| Boundary of Ophir Chasma and Candor Chasma: ESP_065951_1750 ESP_066017_1750 (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 | -4.74 | 287. | 7.75 | -6.57 | 50.0 | 50.3 |
| Candidate Recent Impact Site: ESP_065754_1820 ESP_073681_1820 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.910 | 264. | -5.6 | 4.297 | 55.7 | 57.6 |
| Gully Monitoring and Topography: ESP_065837_1415 ESP_066589_1415 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.0 | 163. | 4.75 | -23.9 | 45.1 | 41.7 |
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