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.
Nirgal Vallis Headwaters: ESP_085046_1530 ESP_085191_1530 (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 | -26.9 | 313. | 8.72 | 25.06 | 36.5 | 36.6 |
Landforms in Utopia Planitia: ESP_085146_2110 ESP_085423_2110 (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 | 30.77 | 96.2 | 7.62 | -4.77 | 52.0 | 49.5 |
Possible Hydrothermal Setting in Northeast Syrtis Major Region: ESP_085160_1970 ESP_085015_1970 (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 | 16.88 | 76.6 | -0.4 | -17.1 | 43.5 | 46.0 |
Crater Wall with Potential Chloride Deposit Outcrop: ESP_084905_1470 ESP_085406_1470 (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 | -32.8 | 205. | -5.5 | 26.95 | 38.6 | 42.1 |
Dark Lanes in South Polar Residual Cap: ESP_085022_0905 ESP_076186_0905 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.2 | 306. | 26.9 | 29.78 | 77.5 | 76.8 |
Raised Glacier-Like Forms in Arabia Terra: ESP_085043_2150 ESP_085109_2150 (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 | 34.67 | 27.6 | 6.88 | -10.0 | 56.2 | 56.3 |
Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084987_1015 ESP_085040_1015 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -78.3 | 140. | 0.12 | -17.6 | 69.3 | 71.3 |
Fan and Ridges in Southern Gale Crater: ESP_085171_1745 ESP_077088_1745 (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 | -5.59 | 137. | 14.5 | -1.72 | 34.1 | 39.5 |
Streamlined Form and Hill in Marte Vallis: ESP_085156_1980 ESP_085433_1980 (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 | 17.73 | 185. | 7.29 | -6.33 | 43.5 | 42.2 |
Hillslope Shapes on Holden Crater Rim: ESP_085006_1550 ESP_085151_1550 (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 | -24.7 | 325. | 2.17 | 18.92 | 36.0 | 35.9 |
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