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.
| East Candor Region: PSP_004410_1735 ESP_012229_1735 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.22 | 290. | 0.51 | -28.0 | 44.7 | 57.4 |
| Margin of South Polar Layered Deposits: PSP_005025_0975 PSP_005262_0975 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.2 | 88.9 | -4.3 | 12.29 | 64.5 | 66.2 |
| Alcove in West Hellas Region: PSP_006753_1425 PSP_010814_1425 (Interval in Earth days: 317) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 45.9 | 0 | -22.6 | 56.4 | 72.8 |
| Avalanche Features of Dune Slip Face Seen in MOC Image R06-00380: PSP_006899_1330 PSP_006965_1330 (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 | -46.7 | 20.1 | 8.63 | -9.75 | 65.3 | 67.4 |
| Small Crater Filled By Deltaic Deposits: PSP_006954_1885 ESP_016250_1885 (Interval in Earth days: 724) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.520 | 312 | -0.3 | -27.7 | 38.5 | 44.0 |
| Light-Toned Layered Rock Outcrop in Ladon Vallis: PSP_006637_1590 ESP_023383_1590 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.8 | 330. | 7.10 | 20.68 | 44.1 | 31.2 |
| Small Valley Delta in Crater Near Maja Valles: PSP_005926_1850 ESP_011279_1850 (Interval in Earth days: 417) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.925 | 301. | -8.3 | 17.11 | 36.4 | 55.6 |
| Interior Layered Deposit Outcrop in Candor Chasma: PSP_005834_1725 ESP_011886_1725 (Interval in Earth days: 471) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.40 | 293. | 6.19 | -9.02 | 32.9 | 57.3 |
| Large Fresh Crater Near Marte Vallis: PSP_006985_2020 PSP_009912_2020 (Interval in Earth days: 228) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.51 | 184. | -2.8 | -22.3 | 39.3 | 50.3 |
| Bright Layers in Columbus Crater: PSP_005429_1510 PSP_005851_1510 (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 | -28.4 | 193. | -4.6 | -17.2 | 34.6 | 38.9 |
Page 855 of 900 (8,995 images) | |||||