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.
| Dissected Wrinkle Ridge Surrounded by Viscous Flows in Elysium Planitia: ESP_016572_1875 ESP_016150_1875 (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 | 7.515 | 157. | 16.0 | 25.58 | 42.9 | 38.9 |
| Ejecta Flow and Obstacle at Arandas Crater: ESP_016776_2225 ESP_016842_2225 (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 | 42.39 | 344. | 4.98 | -9.79 | 41.8 | 43.0 |
| Pristine Channels in Fractured Materials on Crater Floor: ESP_016538_2190 ESP_017171_2190 (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 | 38.77 | 2.06 | 7.68 | -7.08 | 41.1 | 41.9 |
| Crater with Lineated Material on Floor: ESP_016824_1465 ESP_016969_1465 (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 | -33.2 | 124. | -2.9 | 10.86 | 71.0 | 71.5 |
| 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 |
| Chlorides in Dune Materials in Noachis Terra: ESP_016380_1520 ESP_019716_1520 (Interval in Earth days: 260) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 5.67 | -8.5 | 15.10 | 62.3 | 63.2 |
| Well-Preserved Impact Crater on Somewhat Older Crater: ESP_016345_2210 ESP_017624_2210 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.46 | 231. | -0.3 | 11.17 | 42.8 | 40.6 |
| Light-Toned Outcrops in Iani Chaos: ESP_016328_1760 ESP_016473_1760 (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 | -3.82 | 341. | 1.72 | 18.56 | 46.9 | 47.0 |
| Possible Phyllosilicate-Rich Area in Syrtis Major: ESP_016628_2040 ESP_017340_2040 (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 | 23.69 | 68.6 | -7.2 | 6.233 | 41.2 | 42.0 |
| Geologic Contact Between Landslides and Blocky Deposit on Floor of Melas Ch: ESP_016739_1715 ESP_018941_1715 (Interval in Earth days: 172) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.58 | 282. | -8.3 | 8.612 | 54.0 | 57.9 |
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