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.
| Pit Crater Chain Southwest of Arsia Mons: ESP_014077_1660 ESP_058186_1660 (Interval in Earth days: 3437) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 236. | -3.3 | 8.798 | 34.6 | 29.8 |
| Ejecta of Crater Sectioned by Erosion: ESP_013362_1710 ESP_013784_1710 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.89 | 315. | 6.60 | -9.43 | 42.6 | 38.8 |
| 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 |
| 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 |
| Small Rayed Crater in Syrtis Major Planum: ESP_012791_1910 ESP_012857_1910 (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 | 10.67 | 62.2 | 4.22 | -17.8 | 58.5 | 59.5 |
| 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 |
| Remnant of Unusual Looking Material on Plains: ESP_012675_1565 ESP_013743_1565 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 353. | -1.3 | 22.39 | 47.7 | 33.5 |
| Layered Material Exposed on Crater Floor: ESP_013017_2150 ESP_013518_2150 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.69 | 8.85 | 6.51 | 22.48 | 72.6 | 67.8 |
| Fluvial Channel in Crommelin Crater: ESP_013097_1850 ESP_030582_1850 (Interval in Earth days: 1362) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.948 | 349. | -6.8 | 21.51 | 53.5 | 51.0 |
| Recent 10 Kilometer Diameter Crater in Ares Vallis: ESP_013335_1975 ESP_020772_1975 (Interval in Earth days: 580) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.40 | 329. | 1.40 | 17.37 | 58.3 | 58.8 |
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