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.
| Sinuous Ridge and Channel Southwest of Capen Crater: ESP_066990_1850 ESP_067333_1850 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.150 | 12.7 | -2.4 | 7.947 | 44.9 | 41.7 |
| Vent and Channel East of Olympus Mons: ESP_067061_1990 ESP_067404_1990 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.89 | 232. | 5.92 | 17.21 | 51.5 | 47.2 |
| Dune Encroachment on Nereidum Montes Hillslope: ESP_067151_1330 ESP_067283_1330 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.6 | 305. | 5.00 | -10.6 | 45.5 | 48.0 |
| Chryse Chaos: ESP_067005_1940 ESP_066794_1940 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.96 | 321. | 2.33 | -22.6 | 49.3 | 53.3 |
| Gully Monitoring and Topography: ESP_067155_1415 ESP_074132_1415 (Interval in Earth days: 543) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 195. | 5.52 | 26.12 | 41.5 | 49.6 |
| Shallow Channels Entering Collapse Terrain near Orson Welles Crater: ESP_066979_1780 ESP_073877_1780 (Interval in Earth days: 537) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.90 | 313. | -5.2 | 10.09 | 42.0 | 55.8 |
| Charitum Montes: ESP_067138_1275 ESP_066030_1275 (Interval in Earth days: 86) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -52.0 | 302. | -1.7 | -24.1 | 48.8 | 48.4 |
| Auqakuh Vallis: ESP_067054_2125 ESP_084409_2125 (Interval in Earth days: 1352) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.38 | 61.9 | 5.60 | -11.2 | 60.8 | 64.2 |
| Inverted Channel Feature: ESP_067281_1910 ESP_067492_1910 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.84 | 352. | -7.8 | 25.81 | 45.7 | 41.8 |
| Crater Uplift and Ejecta in Tyrrhena Terra: ESP_067054_1760 ESP_067595_1760 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.93 | 67.0 | 3.09 | -11.7 | 40.2 | 40.2 |
Page 199 of 881 (8,805 images) | |||||