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.
| Cratered Cones in Isidis Planitia: PSP_007872_1900 PSP_009586_1900 (Interval in Earth days: 134) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.820 | 85.7 | -6.6 | -23.4 | 45.1 | 52.9 |
| Layering in East Coprates Chasma Wall: PSP_007864_1655 PSP_007508_1655 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 307. | -8.1 | 4.599 | 57.2 | 52.4 |
| Gullies in a Crater Wall: PSP_007977_2385 PSP_008043_2385 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 58.24 | 89.7 | 4.13 | -8.34 | 47.7 | 48.4 |
| Central Peak and Interior of Large Fresh Gullied Crater: PSP_007757_2190 ESP_016618_2190 (Interval in Earth days: 691) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.65 | 341. | 0.54 | -21.6 | 42.0 | 43.7 |
| 3-Kilometer Diameter Crater with Good Bedrock Exposures in Upper Walls: PSP_007892_1865 ESP_079800_1865 (Interval in Earth days: 5603) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.625 | 259. | 4.25 | -7.35 | 45.6 | 54.0 |
| Fault Relays in the Cerberus Fossae: PSP_007645_1885 PSP_007856_1885 (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 | 8.465 | 164. | -5.5 | -23.3 | 43.9 | 46.8 |
| Gullies: PSP_007771_2290 PSP_008061_2290 (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 | 48.73 | 318. | -5.4 | 3.824 | 45.5 | 43.7 |
| Floor and Central Uplift of Mazamba Crater in Thaumasia Planum: PSP_007100_1520 ESP_033248_1520 (Interval in Earth days: 2038) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 290. | -1.6 | -23.6 | 55.6 | 51.8 |
| Big Fresh Crater with a Gullied Central Peak: PSP_007845_2190 PSP_008135_2190 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.53 | 99.2 | -5.6 | 5.818 | 42.3 | 41.1 |
| Slope Streaks Beginning at Stratigraphic Layers: PSP_007473_1850 PSP_008264_1850 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.996 | 181. | -5.4 | 5.46 | 43.6 | 48.7 |
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