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.
| Bend in Jezero Crater Outlet Valley: ESP_069099_1990 ESP_069310_1990 (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 | 18.75 | 78.3 | 3.62 | 19.36 | 46.7 | 46.5 |
| Stratigraphy Exposed in Walls of Hephaestus Fossae: ESP_069071_2020 ESP_063847_2020 (Interval in Earth days: 407) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.82 | 122. | 3.59 | -29.3 | 46.4 | 57.5 |
| Layered Deposits in Jiji Crater: ESP_069102_1890 ESP_069234_1890 (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 | 8.759 | 358. | -1.7 | -29.0 | 48.9 | 52.4 |
| Pyramus Fossae: ESP_069073_2300 ESP_069284_2300 (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 | 49.68 | 64.6 | -8.8 | 1.467 | 52.7 | 50.8 |
| Esker Candidates in Mamers Valles-Ismenius Cavus Region: ESP_069009_2165 ESP_069431_2165 (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 | 36.39 | 13.0 | -4.6 | 21.01 | 48.6 | 46.0 |
| Gully Monitoring: ESP_069049_2225 ESP_069735_2225 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.34 | -0.4 | 3.25 | -13.1 | 49.4 | 49.7 |
| Xanthe Dorsa: ESP_068945_2245 ESP_069420_2245 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.38 | 317. | -4.7 | -25.5 | 51.1 | 51.5 |
| Small Very Fresh Impact Crater: ESP_069148_1645 ESP_069847_1645 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.2 | 185. | -3.7 | 11.79 | 59.1 | 65.1 |
| Layered Deposits on Floor of Tuskagee Crater: ESP_068219_1775 ESP_072703_1775 (Interval in Earth days: 349) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.69 | 323. | 4.08 | 18.72 | 42.7 | 56.0 |
| Very Well-Preserved 900-Meter Northern Plains Crater : ESP_068700_2420 ESP_068687_2420 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 61.49 | 155. | -0.2 | -26.2 | 60.9 | 63.1 |
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