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.
| Exposures of North Polar Layered Deposits with Unconformities: ESP_026901_2600 ESP_028048_2600 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.00 | 23.3 | 0 | 15.02 | 57.0 | 66.2 |
| Lyot Crater Dune Changes: ESP_026664_2305 ESP_026743_2305 (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 | 50.26 | 28.9 | -6.3 | 15.79 | 43.2 | 41.4 |
| Proposed Site for Future Exploration in Cerberus Palus: ESP_026950_1870 ESP_027016_1870 (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 | 6.777 | 146. | 0.08 | -20.2 | 49.8 | 51.5 |
| Possible Phyllosilicates and Fluvial Features Near Hashir Crater: ESP_026649_1835 ESP_028060_1835 (Interval in Earth days: 109) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.323 | 84.8 | -9.5 | 13.24 | 51.7 | 51.4 |
| Fresh Crater: ESP_026951_2200 ESP_027439_2200 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.72 | 113. | 6.96 | -8.41 | 41.3 | 45.2 |
| Eroded Scarp Near Terminus of Valleys on Western Hecates Tholus: ESP_026752_2125 ESP_027029_2125 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.12 | 148. | -3.1 | -21.6 | 41.7 | 44.3 |
| Fresh 5-Kilometer Diameter Crater Near Ophir Catenae: ESP_026773_1695 ESP_044786_1695 (Interval in Earth days: 1404) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.2 | 301. | -6.4 | -23.9 | 59.8 | 59.1 |
| North Polar Linear Dune Changes: ESP_026942_2640 ESP_026692_2640 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.82 | 318. | 14.3 | 0.356 | 59.2 | 59.2 |
| Candidate Future Landing Site in Trouvelot Crater: ESP_026903_1955 ESP_026824_1955 (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 | 15.16 | 347. | 14.7 | -21.9 | 44.9 | 47.7 |
| IR-Distinct Crater: ESP_026619_2285 ESP_027107_2285 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.34 | 176. | 4.39 | -12.0 | 41.7 | 44.9 |
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