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.
| Gullies and Light-Toned Layers in Crater Walls in Terra Cimmeria: ESP_013328_1410 ESP_014185_1410 (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 | -38.6 | 168. | -6.9 | 18.35 | 39.9 | 37.0 |
| Light Toned Fan Deposit with Possible Clays outside Eberswalde Crater: ESP_013454_1560 ESP_013599_1560 (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 | -23.8 | 325. | 2.78 | 18.84 | 37.6 | 34.9 |
| Gullied Crater Wall: ESP_013207_1365 ESP_031180_1365 (Interval in Earth days: 1401) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.0 | 232. | 3.74 | -6.73 | 41.3 | 38.2 |
| 10 Kilometer Diameter Rayed Crater: ESP_012738_1785 ESP_013094_1785 (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 | -1.41 | 70.8 | 2.49 | 14.97 | 53.0 | 48.7 |
| Inverted Terrain in the Mawrth Vallis Region: ESP_013084_2060 ESP_013361_2060 (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 | 25.90 | 341. | 0.94 | -25.7 | 66.4 | 65.7 |
| Dark Deposits in Gullies in Ariadnes Colles: ESP_013341_1455 ESP_013763_1455 (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 | -34.3 | 172. | 2.11 | -11.4 | 38.6 | 36.8 |
| Crater Fill in Noachis Terra: ESP_013663_1315 ESP_021601_1315 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.1 | 23.9 | -1.3 | 24.37 | 40.9 | 44.5 |
| Possible Monohydrated Sulfate-Rich Terrain in Columbus Crater: ESP_014039_1510 ESP_021832_1510 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.7 | 194. | 7.74 | 26.60 | 33.9 | 38.3 |
| Incipient Scalloped Terrain in Mid-Latitude Mantle at Peneus Patera: ESP_013029_1235 ESP_013306_1235 (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 | -56.1 | 54.6 | -0.3 | -19.2 | 47.7 | 46.9 |
| Gullied Trough Wall: ESP_012602_1415 ESP_013881_1415 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 188. | 6.27 | 18.92 | 48.1 | 35.6 |
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