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.
Repeated Sulfate and Clay Beds in West Gale Crater: ESP_017786_1745 ESP_017931_1745 (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 | -5.36 | 137. | -13. | 1.249 | 57.9 | 57.2 |
Flow Into Breached Crater in Central Elysium Planitia: ESP_018062_1810 ESP_018484_1810 (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 | 0.837 | 160. | -8.0 | -21.3 | 54.3 | 55.6 |
Blocky Flow with Light-Toned Outcrops in Noctis Region: ESP_017834_1720 ESP_018546_1720 (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 | -7.90 | 266. | -5.6 | 11.69 | 59.0 | 58.0 |
Central Uplift of Impact Crater in Tyrrhena Terra: ESP_017748_1665 ESP_026108_1665 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 93.8 | 8.34 | 24.74 | 61.6 | 57.7 |
Ridges and Flow-Like Forms: ESP_017734_2075 ESP_071880_2075 (Interval in Earth days: 4219) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.32 | 111. | -1.2 | 16.1 | 42.7 | 47.9 |
Layered Terrain in Aeolis and Zephyria Regions: ESP_017825_1760 ESP_018458_1760 (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 | -3.75 | 149. | 13.9 | -9.22 | 55.2 | 57.1 |
Rampart Crater Ejecta Exposed in Cross-Section: ESP_018017_1680 ESP_026799_1680 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.1 | 310. | -0.4 | 10.24 | 61.6 | 60.0 |
Cones at Edge of North Polar Layered Deposits: ESP_017885_2595 ESP_018004_2595 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.12 | 285. | 13.2 | -3.67 | 55.5 | 56.7 |
Fault in Ius Chasma: ESP_017939_1720 ESP_025231_1720 (Interval in Earth days: 568) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.89 | 279. | -3.1 | -22.3 | 59.0 | 50.2 |
Raised Polygonal Ridges and Light-Toned Material in Syrtis Region: ESP_018065_1975 ESP_019133_1975 (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 | 17.49 | 76.4 | -5.2 | 15.52 | 46.5 | 48.0 |
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