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.
| Faulted Plains in Tempe Terra: ESP_034791_2245 ESP_035081_2245 (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 | 44.15 | 271. | 6.29 | 23.09 | 41.3 | 39.7 |
| Floor of East Candor Chasma: ESP_034685_1730 ESP_034751_1730 (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 | -6.78 | 292. | 11.1 | -13.5 | 53.9 | 56.0 |
| Airy Crater Dune Changes: ESP_034643_1750 ESP_035065_1750 (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 | -5.04 | 0.09 | -4.8 | -25.3 | 53.7 | 57.6 |
| Layered Deposits in Bulhar Crater: ESP_034585_2305 ESP_035996_2305 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.42 | 134. | 7.73 | -7.45 | 43.2 | 46.4 |
| InSight Mission Candidate Landing Site: ESP_034717_1840 ESP_035561_1840 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.854 | 137. | 12.2 | -20.8 | 48.1 | 53.9 |
| Candidate Future Landing Site: ESP_034802_1525 ESP_034868_1525 (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 | -27.4 | 341. | -4.0 | -25.0 | 69.5 | 71.2 |
| Domoni Crater Secondaries: ESP_034832_2300 ESP_035887_2300 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.69 | 231. | 0.40 | -18.2 | 43.0 | 46.5 |
| Sinuous Ridge with Mesa at Terminus in Kasabi Crater: ESP_034508_1520 ESP_035154_1520 (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 | -27.7 | 89.1 | -6.1 | 19.81 | 67.4 | 70.3 |
| Channels on Mesa in Southern Elysium Planitia: ESP_034558_1775 ESP_052307_1775 (Interval in Earth days: 1383) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.48 | 159. | 6.18 | 26.96 | 50.8 | 47.7 |
| Lava Textures inside Kasei Valles: ESP_034724_2065 ESP_035568_2065 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.17 | 303. | 4.53 | -23.0 | 41.0 | 45.8 |
Page 473 of 877 (8,766 images) | |||||