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.
| Light-Toned Stratified Materials in Melas Chasma: ESP_027657_1680 ESP_028567_1680 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 287. | 10.8 | -2.34 | 59.3 | 57.4 |
| Candidate Future Landing Site North of Hellas Planitia: ESP_027481_1540 ESP_025714_1540 (Interval in Earth days: 137) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.8 | 54.6 | 3.40 | -6.59 | 68.7 | 65.5 |
| Small Crater on North Polar Deposits: ESP_027496_2620 ESP_027470_2620 (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 | 81.83 | 333. | 6.09 | -8.57 | 61.5 | 62.1 |
| Degraded Crater in Utopia Planitia: ESP_027743_2305 ESP_028033_2305 (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 | 49.95 | 92.8 | -1.2 | 23.84 | 49.2 | 50.3 |
| Survey Layering and Faulting in Layered Deposits in Melas Chasma: ESP_027446_1670 ESP_027723_1670 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 288. | -1.0 | -18.0 | 60.7 | 61.2 |
| Capri Chasma: ESP_027564_1655 ESP_053818_1655 (Interval in Earth days: 2046) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.5 | 308. | -4.4 | 5.774 | 61.8 | 60.3 |
| Sinus Meridiani Dune Changes: ESP_027443_1815 ESP_028142_1815 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.630 | 8.40 | 4.32 | -9.06 | 52.5 | 53.8 |
| North Polar Gypsum Dune Changes: ESP_027606_2605 ESP_027580_2605 (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 | 80.11 | 212. | 8.52 | -8.75 | 61.3 | 62.1 |
| Possible Chloride-Rich Terrain: ESP_027406_1485 ESP_036333_1485 (Interval in Earth days: 696) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.4 | 303. | -7.3 | 15.19 | 73.3 | 72.7 |
| Complex Superposition of Fractures: ESP_027486_2240 ESP_027631_2240 (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 | 43.43 | 269. | -1.1 | 13.86 | 45.3 | 45.2 |
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