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.
| Coprates Chasma Dune Changes: ESP_062153_1660 ESP_062219_1660 (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 | -13.9 | 296. | -1.0 | -25.8 | 62.1 | 63.9 |
| Dunes Dubbed Carlsbad: ESP_062187_2800 ESP_062451_2800 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.99 | 270. | -8.3 | 6.392 | 70.5 | 70.2 |
| Ice-Filled North Polar Layered Deposit Crater: ESP_062014_2645 ESP_062053_2645 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.22 | 98.3 | -2.3 | 11.61 | 59.6 | 59.2 |
| Mesa in Chryse Planitia: ESP_061954_1990 ESP_062020_1990 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.95 | 324. | 8.90 | -8.79 | 43.5 | 45.1 |
| Mound in Holden Crater: ESP_061875_1545 ESP_062152_1545 (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 | -25.2 | 326. | 14.4 | -8.23 | 68.6 | 70.2 |
| Flow Margin in Phlegra Dorsa: ESP_061854_2080 ESP_061920_2080 (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 | 27.85 | 173. | 8.37 | -7.74 | 40.8 | 42.4 |
| Channel Near Moreux Crater: ESP_061951_2210 ESP_062241_2210 (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 | 40.51 | 43.6 | 6.27 | 24.54 | 40.5 | 39.8 |
| Dunes Dubbed San Onofre: ESP_062181_2610 ESP_062207_2610 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.99 | 231. | -7.8 | 7.521 | 58.1 | 57.3 |
| Crater in Arabia Terra: ESP_062137_2140 ESP_061781_2140 (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 | 33.62 | 5.22 | 21.4 | 6.959 | 39.8 | 40.0 |
| Layered Cone in Crater in Cydonia Region: ESP_062019_2225 ESP_062309_2225 (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 | 42.27 | 348. | -4.4 | 9.982 | 41.8 | 41.8 |
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