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.
| Phlegra Montes: ESP_066483_2155 ESP_084603_2155 (Interval in Earth days: 1412) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.23 | 164. | -2.4 | -12.5 | 70.4 | 63.8 |
| Impact on South Polar Layered Deposits: ESP_066101_0980 ESP_066220_0980 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.1 | 175. | 8.05 | -6.00 | 61.2 | 62.2 |
| Athabasca Valles Distributary: ESP_066035_1875 ESP_057978_1875 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.385 | 153. | 7.18 | -7.96 | 55.4 | 42.4 |
| Center of Crommelin Crater: ESP_065830_1850 ESP_057641_1850 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.944 | 349. | -8.4 | 6.362 | 56.8 | 44.2 |
| Ostrov Crater Fans: ESP_065778_1530 ESP_066543_1530 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.4 | 331. | 4.24 | 27.83 | 46.0 | 36.6 |
| South Polar Cap Vertical Change Monitoring: ESP_065909_0930 ESP_065989_0930 (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 | -86.7 | 16.2 | 23.3 | 8.954 | 63.8 | 64.7 |
| Leveed Candidate Mudflow: ESP_065910_1995 ESP_066042_1995 (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 | 19.36 | 323. | 1.75 | -22.4 | 63.9 | 64.6 |
| Candidate Recent Impact Site: ESP_065754_1820 ESP_073681_1820 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.910 | 264. | -5.6 | 4.297 | 55.7 | 57.6 |
| Elongated Collapse Pit in Ceraunius Fossae: ESP_066005_2110 ESP_074143_2110 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.54 | 250. | -3.7 | -15.7 | 71.0 | 72.0 |
| Gullies and Crater Fill: ESP_065798_1430 ESP_066220_1430 (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 | -36.8 | 148. | -4.5 | 27.39 | 46.2 | 39.2 |
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