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.
Seasonal Monitoring Candidate: ESP_013787_0955 ESP_014037_0955 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.4 | 274. | -7.7 | 8.965 | 66.4 | 67.8 |
Steep Lobate Scarps in Kasei Valles: ESP_012717_1910 ESP_013139_1910 (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 | 10.88 | 282. | 2.07 | -8.93 | 59.1 | 56.6 |
Multi-Aprons of Ganges Region Landslide: ESP_013217_1715 ESP_013718_1715 (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 | -8.33 | 315. | -5.3 | 17.64 | 45.4 | 37.8 |
South Polar Layered Deposits Exposed in Ultimum Chasma: ESP_013778_0985 ESP_013659_0985 (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 | -81.2 | 147. | -12. | 4.816 | 63.8 | 61.6 |
Crater Fill in Noachis Terra: ESP_013663_1315 ESP_021601_1315 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.1 | 23.9 | -1.3 | 24.37 | 40.9 | 44.5 |
Possible Monohydrated Sulfate-Rich Terrain in Columbus Crater: ESP_014039_1510 ESP_021832_1510 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.7 | 194. | 7.74 | 26.60 | 33.9 | 38.3 |
Recent Gullies in a Crater in Noachis Terra: ESP_013222_1410 ESP_013288_1410 (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 | -38.8 | 182. | 0.69 | -18.8 | 40.4 | 41.3 |
Contact between Parallel Bedded and Contorted Layers in South Melas Region: ESP_012862_1685 ESP_013930_1685 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 286. | 1.87 | 24.04 | 48.0 | 34.2 |
Fractured Lava Dome in Eastern Tharsis Region: ESP_013904_1970 ESP_013970_1970 (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 | 16.62 | 275. | -4.7 | -25.2 | 51.1 | 51.6 |
Exposure of Polar Layered Deposits Not Well Observed: ESP_013886_0875 ESP_022748_0875 (Interval in Earth days: 691) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.4 | 165. | 4.63 | 10.95 | 71.0 | 71.9 |
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