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.
| Flow Deposits in Eastern Ladon Valles: ESP_062099_1620 ESP_062534_1620 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.9 | 332. | -6.1 | 19.86 | 65.0 | 63.4 |
| Clay-Bearing Landslide and Outcrop in Degraded Crater: ESP_061990_1770 ESP_062056_1770 (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 | -2.77 | 65.1 | 5.98 | -13.8 | 54.3 | 55.8 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_061950_1990 ESP_062095_1990 (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 | 18.67 | 77.4 | -27. | -11.1 | 46.6 | 45.5 |
| 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 |
| Ice-Filled Crater in North Polar Layered Deposits: ESP_062085_2645 ESP_062203_2645 (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 | 84.40 | 315. | 0.89 | 14.85 | 59.7 | 59.7 |
| 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 |
| Dunes Dubbed La Jolla: ESP_062168_2585 ESP_062115_2585 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.19 | 229. | -8.3 | 6.672 | 56.4 | 55.3 |
| Crater Rim in Cydonia Mensae: ESP_062098_2165 ESP_061742_2165 (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 | 36.07 | 351. | 10.5 | -7.44 | 40.5 | 41.1 |
| 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 |
| 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 |
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