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.
| Well-Preserved Impact Crater: ESP_013238_1945 ESP_013871_1945 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.53 | 98.5 | -0.1 | -22.9 | 57.4 | 51.3 |
| 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 |
| South Polar Layered Deposits Exposed in Promethei Lingula: ESP_013832_0975 ESP_013647_0975 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.5 | 112. | -3.5 | 14.29 | 64.8 | 62.0 |
| Rootless Cones in Isidis Planitia: ESP_013212_1890 ESP_020082_1890 (Interval in Earth days: 536) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.729 | 88.8 | 2.89 | 20.63 | 53.9 | 52.9 |
| 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 |
| 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 |
| 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 |
| 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 |
| 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 |
| Layering in Argyre Planitia Sinuous Ridge: ESP_012927_1245 ESP_013626_1245 (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 | -55.1 | 318. | 1.77 | -23.3 | 48.2 | 46.0 |
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