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.
| Possible Kieserite-Rich Terrain in Hebes Chasma: ESP_014418_1790 ESP_019864_1790 (Interval in Earth days: 425) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.18 | 284. | 1.76 | -16.7 | 35.6 | 56.2 |
| Tractus Catena: ESP_014432_2110 ESP_023135_2110 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.77 | 257. | 5.46 | -19.5 | 53.6 | 55.4 |
| Well-Preserved 7-Kilometer Diameter Gullied Crater in Newton Region: ESP_014395_1425 ESP_022188_1425 (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 | -37.2 | 198. | -8.2 | 9.964 | 39.9 | 36.2 |
| Fans and Polygons: ESP_014266_0925 ESP_014410_0925 (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 | -87.3 | 167. | 8.77 | 22.08 | 73.6 | 74.6 |
| Large Rocky Central Uplift: ESP_014410_1470 ESP_020423_1470 (Interval in Earth days: 468) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.5 | 146. | 2.49 | -12.5 | 37.2 | 60.1 |
| Megabreccia and Layered Deposits in Holden Crater: ESP_014443_1530 ESP_022724_1530 (Interval in Earth days: 646) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.6 | 325. | 0.41 | -14.1 | 35.4 | 33.6 |
| Triple Crater Fill and Gullies: ESP_014263_1435 ESP_014329_1435 (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 | -36.0 | 199. | 14.3 | -4.42 | 36.7 | 38.5 |
| Basal Scarp of South Polar Layered Deposits: ESP_014424_1070 ESP_022837_1070 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -72.7 | 135. | -1.5 | -21.0 | 64.2 | 59.4 |
| Exposures of Layered Rocks in Argyre Region: ESP_014167_1300 ESP_021947_1300 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.7 | 302. | 8.10 | -18.2 | 43.7 | 44.1 |
| Ferric Oxide-Rich Deposit in East Candor Chasma: ESP_014154_1730 ESP_014431_1730 (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 | -6.75 | 292. | 5.69 | -21.1 | 35.2 | 35.9 |
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