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.
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088171_2295 ESP_088395_2295 (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 | 49.11 | 309. | -5.5 | 19.83 | 44.5 | 42.6 |
| Channel South of Janssen Crater: ESP_088168_1800 ESP_088458_1800 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.118 | 37.6 | -7.2 | 12.15 | 55.4 | 54.8 |
| Pits in North Polar Layered Deposits: ESP_088394_2650 ESP_088367_2650 (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 | 84.81 | 318. | -7.7 | 6.46 | 60.4 | 59.8 |
| Dune Field: ESP_088070_2535 ESP_088413_2535 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.41 | 178. | 0.65 | -15.8 | 53.4 | 54.6 |
| Kasei Valles Scarps and Terraces: ESP_088145_2055 ESP_088567_2055 (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 | 25.39 | 302. | -3.6 | -28.6 | 44.6 | 48.0 |
| Meander in Channel Southwest of Mamers Valles: ESP_088327_2165 ESP_088538_2165 (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 | 35.99 | 10.3 | 4.70 | -6.95 | 42.9 | 44.4 |
| Dune Survey: ESP_088162_2540 ESP_088676_2540 (Interval in Earth days: 41) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.92 | 186. | -0.7 | 14.11 | 53.6 | 53.3 |
| Obstacle within Lobate Debris Apron: ESP_088359_1435 ESP_088570_1435 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.0 | 225. | 7.68 | -5.73 | 78.9 | 79.8 |
| Monitor Slope in West Coprates Chasma: ESP_088106_1685 ESP_088673_1685 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.5 | 290. | 5.12 | -16.4 | 61.5 | 63.9 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088230_2400 ESP_088454_2400 (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 | 59.81 | 135. | -4.2 | 14.96 | 47.5 | 46.2 |
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