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.
| Pitted and Fractured Surfaces in Southern Mojave Region: ESP_014034_1870 ESP_014311_1870 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.105 | 327. | 0.98 | -24.4 | 43.1 | 41.9 |
| Terby Crater Surroundings: ESP_013885_1520 ESP_020465_1520 (Interval in Earth days: 513) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.9 | 79.1 | 4.84 | -7.13 | 34.3 | 58.0 |
| Gullies: ESP_012734_1265 ESP_012879_1265 (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 | -53.1 | 188. | -7.8 | 2.791 | 50.7 | 47.9 |
| Active Geyser Locale: ESP_014083_0945 ESP_014122_0945 (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 | -85.4 | 103. | 8.28 | 22.35 | 69.3 | 68.8 |
| Gullies and Lobate Material in a Crater in the Nereidum Montes: ESP_014127_1420 ESP_020786_1420 (Interval in Earth days: 519) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.5 | 314. | -2.1 | 19.93 | 37.6 | 54.3 |
| Possible Cyclic Bedding in Arabia Terra: ESP_013611_1910 ESP_014033_1910 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.87 | 355. | 0.61 | -17.2 | 50.8 | 46.6 |
| Strike Slip Fault in Amazonis Planitia: ESP_012944_1985 ESP_013221_1985 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.44 | 204. | 2.77 | -22.9 | 62.2 | 61.7 |
| Scarp Likely Exposing Polar Layered Deposits in Area Not Well Observed: ESP_013910_0880 ESP_022641_0880 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 216. | 8.73 | 19.64 | 70.6 | 70.3 |
| Central Pit Gullies in Asimov Crater: ESP_013123_1330 ESP_013268_1330 (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 | -46.8 | 4.93 | 13.8 | 22.63 | 42.3 | 40.3 |
| Well Preserved 20 Kilometer Diameter Impact Crater: ESP_013684_1455 ESP_020910_1455 (Interval in Earth days: 563) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 168. | -2.8 | 19.71 | 36.4 | 51.7 |
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