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.
| Raised Polygonal Ridges and Light-Toned Material in Syrtis Region: ESP_018065_1975 ESP_019133_1975 (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 | 17.49 | 76.4 | -5.2 | 15.52 | 46.5 | 48.0 |
| Light-Toned Outcrops in Noctis Region: ESP_017979_1715 ESP_018401_1715 (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 | -8.26 | 267. | -7.1 | -21.7 | 59.6 | 60.6 |
| Mounds and Polygonal Features in Crater: ESP_018078_2445 ESP_018210_2445 (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 | 64.31 | 70.3 | 10.5 | -7.11 | 48.1 | 50.0 |
| Valley-Crater Intersection with Exposed Layers: ESP_018055_2120 ESP_018899_2120 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.60 | 346. | 3.16 | -20.2 | 42.5 | 48.6 |
| Exposures of Various North Polar Geologic Units: ESP_017845_2625 ESP_018016_2625 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.42 | 302. | -5.5 | 9.318 | 58.6 | 58.2 |
| Cones at Edge of North Polar Layered Deposits: ESP_017885_2595 ESP_018004_2595 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.12 | 285. | 13.2 | -3.67 | 55.5 | 56.7 |
| Small Rayed Crater in Elysium Planitia: ESP_017785_1975 ESP_018418_1975 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.20 | 160. | 5.75 | -15.8 | 45.1 | 48.3 |
| Clay Diversity on Flank of Mawrth Vallis: ESP_017897_2045 ESP_018530_2045 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.08 | 341. | 4.44 | -14.5 | 43.4 | 46.8 |
| Impact Crater Teetering on the Edge of a Canyon: ESP_017740_1680 ESP_025810_1680 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.7 | 312. | 5.84 | -8.97 | 60.6 | 56.8 |
| Northern Hemisphere Gullies on a West-Facing Crater Slope: ESP_017405_2270 ESP_017827_2270 (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 | 46.67 | 90.1 | 7.09 | -4.59 | 41.7 | 43.0 |
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