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.
| Mounds and Pit on Thick Carbon Dioxide Ice: ESP_075399_0920 ESP_074989_0920 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.1 | 219. | 15.6 | 25.47 | 66.9 | 64.0 |
| Canyon Floor in East Coprates Chasma: ESP_075407_1650 ESP_075473_1650 (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 | -15.0 | 304. | -4.1 | -21.8 | 38.2 | 39.0 |
| Layers at Edge of Pedestal Crater in Tikhonravov Crater: ESP_075364_1940 ESP_076353_1940 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.64 | 35.2 | -7.3 | 2.427 | 53.3 | 41.6 |
| Channel and Crater North of Huygens Crater: ESP_075416_1745 ESP_075772_1745 (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 | -5.39 | 57.5 | 0.14 | 18.63 | 41.3 | 36.4 |
| Extra-Crater Sinuous Ridge: ESP_075462_1065 ESP_075594_1065 (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 | -73.4 | 255. | 2.18 | -8.96 | 56.9 | 58.7 |
| Coprates Chasma: ESP_075486_1655 ESP_075908_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 | -14.1 | 307. | 4.94 | -8.37 | 37.0 | 35.4 |
| Steep-Front Deposit with Light-Toned Layers in Northern Arabia Terra: ESP_075497_2135 ESP_084187_2135 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.37 | 2.44 | -7.0 | 3.051 | 65.9 | 67.0 |
| Mesa in Southern Utopia Planitia: ESP_075480_2035 ESP_084025_2035 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.41 | 107. | -1.6 | 13.08 | 58.3 | 60.9 |
| Eastern Rim of Hadley Crater and Surrounding Terrain: ESP_075386_1610 ESP_076230_1610 (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 | -18.5 | 157. | 5.64 | -8.90 | 36.8 | 35.8 |
| Small Channel South of Mangala Valles: ESP_074883_1600 ESP_083059_1600 (Interval in Earth days: 637) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.6 | 209. | 6.85 | -7.00 | 42.0 | 51.1 |
Page 148 of 891 (8,901 images) | |||||