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.
| Gullies in Crater North of Iani Chaos: ESP_026956_1800 ESP_027523_1800 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.120 | 345. | -21. | -2.25 | 54.9 | 53.7 |
| Northern Plains Cratered Cones in Acidalia Planitia: ESP_026732_2215 ESP_027431_2215 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.15 | 333. | -4.3 | -20.7 | 41.7 | 46.5 |
| Cones at Edge of North Polar Layered Deposits: ESP_026905_2610 ESP_027024_2610 (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 | 80.71 | 267. | 8.70 | -5.21 | 57.0 | 58.2 |
| Fresh Impact Crater: ESP_026661_1495 ESP_062977_1490 (Interval in Earth days: 2830) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.2 | 120. | 3.50 | -8.29 | 72.9 | 72.0 |
| Crater Inside Athabasca Valles: ESP_026620_1880 ESP_026686_1880 (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 | 8.237 | 154. | 7.94 | -13.7 | 47.9 | 49.7 |
| Light-Tone Material Crater Wall in CTX Image G02_019002_1586_XN_21S300W: ESP_026861_1555 ESP_027349_1555 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.0 | 59.4 | 5.54 | -17.1 | 68.5 | 69.1 |
| Very Well-Preserved Impact Crater on Northern Plains: ESP_026828_2420 ESP_026907_2420 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 61.68 | 228. | -3.4 | 13.20 | 47.2 | 46.2 |
| Candidate Future Landing Site Near Sabrina Vallis: ESP_026812_1920 ESP_026878_1920 (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 | 11.75 | 313. | -1.3 | -21.3 | 47.4 | 49.1 |
| Crater on Northern Plains: ESP_026880_2355 ESP_026959_2355 (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 | 55.32 | 253. | -20. | -1.45 | 46.5 | 45.1 |
| Dunes and North Polar Outlier: ESP_026634_2595 ESP_026528_2595 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.16 | 125. | -21. | 5.115 | 57.5 | 55.7 |
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