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.
| Chaos on the Floor of Candor Chasma: ESP_016686_1735 ESP_017108_1735 (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 | -6.49 | 287. | 10.2 | -4.71 | 51.1 | 55.2 |
| Phyllosilicate-Rich Terrain in Degraded Crater: ESP_016580_1865 ESP_019837_1865 (Interval in Earth days: 254) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.503 | 300. | 0 | -14.0 | 44.6 | 54.9 |
| Fresh Multiple Impact: ESP_016718_2005 ESP_018353_2005 (Interval in Earth days: 127) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.26 | 131. | 0.06 | 15.40 | 41.3 | 44.6 |
| Zunil Crater Secondary Crater Cluster: ESP_016796_1830 ESP_016941_1830 (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 | 2.871 | 164. | -8.6 | 7.724 | 48.3 | 48.1 |
| Small Crater Exposed in Cross-Section by Erosion: ESP_016699_1715 ESP_019178_1715 (Interval in Earth days: 193) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.45 | 293. | 1.41 | -13.7 | 52.9 | 58.8 |
| Possible Landing Site for MSL in Eastern Margaritifer Terra: ESP_016499_1745 ESP_016565_1745 (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 | -5.60 | 353. | -7.2 | -27.6 | 50.0 | 52.2 |
| Outcrop of Rhythmic Bedding in Arabia Terra: ESP_016657_1890 ESP_017013_1890 (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 | 8.820 | 358. | -1.3 | 8.534 | 44.4 | 45.7 |
| Discontinuous Small Channel South of Dao Vallis: ESP_016311_1420 ESP_016588_1420 (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 | -37.6 | 89.5 | 5.56 | -17.0 | 67.7 | 72.4 |
| Impact Monitoring Site in Utopia Planitia: ESP_016495_2240 ESP_028666_2240 (Interval in Earth days: 949) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.65 | 96.3 | -3.2 | 7.185 | 43.5 | 58.5 |
| Dissected Terrain in Arcadia Planitia: ESP_016492_2175 ESP_017125_2175 (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 | 37.02 | 178. | 1.71 | -12.6 | 41.3 | 42.2 |
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