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.
| The 2-Kilometer Diameter Well-Preserved Vaduz Crater: ESP_023302_2185 ESP_023579_2185 (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 | 38.23 | 15.8 | 1.32 | -22.4 | 57.8 | 55.3 |
| Proposed MSR Landing Site in Jezero Crater: ESP_023102_1985 ESP_023168_1985 (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 | 18.34 | 77.7 | 8.20 | -11.8 | 45.2 | 45.6 |
| Possible Future Landing Site Near Mawrth Vallis: ESP_023343_2050 ESP_023633_2050 (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 | 24.51 | 338. | -1.3 | 19.90 | 47.1 | 42.4 |
| Intracrater Dunes: ESP_023269_1075 ESP_023401_1075 (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 | -72.0 | 214. | 2.08 | -12.9 | 63.4 | 66.3 |
| Small Mounds in Chryse Planitia: ESP_023159_1995 ESP_023225_1995 (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 | 19.36 | 322. | -2.4 | -20.9 | 45.9 | 46.3 |
| Layered Material in Melas Chasma: ESP_023266_1690 ESP_032035_1690 (Interval in Earth days: 683) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.8 | 284. | 0.87 | -12.1 | 31.5 | 33.0 |
| Channel in Cerberus Region: ESP_023310_1870 ESP_023600_1870 (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 | 7.005 | 161. | -1.4 | 23.90 | 36.8 | 33.0 |
| Light-Toned Unit along Noctis Labyrinthus Plains: ESP_023425_1700 ESP_024137_1700 (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 | -10.0 | 264. | -5.4 | 13.39 | 32.1 | 35.7 |
| Dune Changes in Green Crater: ESP_023145_1270 ESP_022855_1270 (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 | -52.6 | 351. | 20.8 | -0.20 | 45.6 | 43.7 |
| Tongue-Shaped Flow Feature in Hellas Montes Region: ESP_023141_1435 ESP_023642_1435 (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 | -36.0 | 101. | -5.7 | 15.39 | 37.1 | 41.8 |
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