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.
| Dunes Dubbed Newport: ESP_062824_2560 ESP_062666_2560 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 75.89 | 314. | 5.37 | -9.62 | 58.6 | 58.2 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_062741_1990 ESP_063387_1990 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.68 | 77.2 | 0.54 | 17.50 | 47.1 | 49.4 |
| Possible Equatorial Ice-Rich Material in Schiaparelli Crater: ESP_062717_1755 ESP_062862_1755 (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 | -4.47 | 16.2 | -8.8 | 1.672 | 57.2 | 56.5 |
| Northern Mid-Latitude Crater: ESP_062806_2150 ESP_062740_2150 (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 | 34.80 | 100. | -3.6 | 15.57 | 45.8 | 43.6 |
| Flow Deposits in Eastern Ladon Valles Basin: ESP_062745_1615 ESP_062956_1615 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.2 | 332. | 8.06 | -7.02 | 64.1 | 64.6 |
| Sinuous Inverted Channel in Large Basin in East Arabia Terra: ESP_062808_2085 ESP_062874_2085 (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 | 28.26 | 45.7 | 8.60 | -12.7 | 45.0 | 47.3 |
| Dunes with Furrows: ESP_062912_2575 ESP_053918_2575 (Interval in Earth days: 701) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.16 | 75.5 | -7.2 | 7.214 | 61.0 | 58.0 |
| Terraced Fan in East Candor Chasma: ESP_062786_1730 ESP_062997_1730 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.84 | 292. | -3.2 | -17.8 | 58.1 | 59.1 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_062662_1990 ESP_062952_1990 (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 | 18.61 | 77.2 | -29. | -12.5 | 49.4 | 49.2 |
| High-Latitude Crater with Patterned Ground: ESP_062992_2475 ESP_063216_2475 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.07 | 55.0 | -2.5 | 13.10 | 56.3 | 57.9 |
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