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.
| Tilted Mesas Near Athabasca Valles: ESP_035033_1880 ESP_054061_1880 (Interval in Earth days: 1482) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.762 | 149. | 8.28 | 24.88 | 48.0 | 46.6 |
| Light-Toned Deposits along Coprates Chasma Wallrock: ESP_034975_1670 ESP_034329_1670 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.8 | 296. | -0.1 | -22.9 | 60.3 | 57.0 |
| Relatively Unmantled Pole-Facing Gullies: ESP_035080_2185 ESP_035370_2185 (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 | 38.16 | 303. | -3.3 | 18.49 | 41.6 | 40.2 |
| Domoni Crater Secondaries: ESP_034990_2335 ESP_035425_2335 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.10 | 236. | 2.93 | 25.72 | 43.7 | 41.8 |
| Insight Mission Candidate Landing Site: ESP_035073_1840 ESP_036550_1840 (Interval in Earth days: 115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.766 | 136. | 21.7 | -2.21 | 49.2 | 53.9 |
| Textured Materials in Northwest Hellas Planitia: ESP_034905_1380 ESP_035406_1380 (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 | -41.4 | 51.4 | -2.7 | 14.35 | 80.3 | 81.4 |
| Candidate Landing Site for 2020 Mission in Nili Patera: ESP_035247_1890 ESP_035537_1890 (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 | 9.027 | 67.4 | -2.7 | 27.45 | 49.1 | 47.5 |
| Floor of East Candor Chasma: ESP_035041_1720 ESP_043441_1720 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.73 | 295. | -23. | 2.251 | 59.0 | 53.3 |
| Candidate Landing Site for 2020 Mission in Gusev Crater: ESP_035230_1655 ESP_035586_1655 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.5 | 175. | -13. | -3.85 | 63.4 | 63.6 |
| Falling Dunes along Eastern Coprates Chasma Massif: ESP_035278_1655 ESP_034856_1655 (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 | -14.3 | 303. | -0.3 | 17.51 | 62.6 | 59.5 |
Page 466 of 877 (8,766 images) | |||||