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.
| Hydrated Minerals and Gully on Central Uplift of Li Fan Crater: ESP_013564_1330 ESP_013709_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 | 207. | -5.9 | 5.732 | 40.8 | 39.9 |
| Gullies in Dunes: ESP_014151_1325 ESP_021509_1325 (Interval in Earth days: 573) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.1 | 19.5 | 5.65 | -10.1 | 42.1 | 48.1 |
| Light-Toned Outcrops along Ius Region Wallrock: ESP_012849_1705 ESP_013126_1705 (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 | -9.22 | 281. | -3.9 | -28.8 | 49.2 | 48.0 |
| Steep Shields in Tharsis Region: ESP_014037_1760 ESP_014182_1760 (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 | -3.90 | 246. | -1.4 | 16.04 | 37.7 | 35.2 |
| Enigmatic Pit in Southern Cerberus Palus: ESP_012893_1775 ESP_013605_1775 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.47 | 160. | -6.3 | 12.12 | 51.7 | 42.2 |
| Tongue-Shaped Features within Alcoves on South Mid-Latitude Crater Wall: ESP_014058_1450 ESP_014335_1450 (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 | -34.5 | 37.1 | 1.29 | -21.3 | 36.0 | 39.2 |
| 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 |
| Distal Ramparts for Fresh Crater Santa Fe in Chryse Planitia: ESP_012795_1995 ESP_013639_1995 (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 | 19.03 | 312. | -0.8 | -24.0 | 63.6 | 57.4 |
| Gullies: ESP_012722_1400 ESP_012867_1400 (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 | -39.6 | 153. | -6.2 | 7.111 | 47.5 | 44.4 |
| Fluidized Ejecta in the Kasei Valles Region: ESP_013204_2060 ESP_083253_2060 (Interval in Earth days: 5458) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.76 | 305. | 0 | 16.06 | 65.4 | 67.6 |
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