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.
| Possible MSL Landing Site in Gale Crater: ESP_011417_1755 ESP_011562_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 | -4.44 | 137. | -15. | 1.284 | 58.8 | 57.4 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010555_2720 PSP_010583_2680 (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 | 87.91 | 156. | -8 | -8.54 | 75.6 | 75.2 |
| Central Peak of Gale Crater: PSP_010428_1745 ESP_016085_1745 (Interval in Earth days: 440) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.40 | 137. | 4.52 | -23.3 | 57.8 | 46.9 |
| Giza Region Stereo: ESP_011447_0950 ESP_011448_0950 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.8 | 65.7 | 9.42 | -17.5 | 86.7 | 89.1 |
| Especially Bright Materials in Candor Chasma: ESP_011372_1730 ESP_012295_1730 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.78 | 284. | 5.39 | 20.7 | 57.4 | 53.0 |
| The North Pole of Mars: PSP_010545_2700 PSP_010586_2700 (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 | 89.98 | -154 | -25. | -25.6 | 76.8 | 77.4 |
| Floor of Sirenum Region Crater: ESP_011494_1535 ESP_011639_1535 (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 | -26.0 | 199. | -26. | -12.0 | 62.7 | 60.3 |
| Crater in Icaria Fossae Region with Intersecting Graben: ESP_011440_1335 ESP_011941_1335 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.9 | 234. | -5.1 | 15.24 | 68.4 | 59.6 |
| Very Recent Small Crater: PSP_010772_2145 ESP_045136_2145 (Interval in Earth days: 2678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.38 | 100. | 4.13 | -8.37 | 54.7 | 42.8 |
| Well-Preserved Impact Crater on Northern Plains: PSP_010559_2170 ESP_016005_2170 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.54 | 155. | 5.58 | -8.20 | 52.5 | 43.4 |
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