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.
| Eastern Portion of Small Melas Chasma Basin: ESP_017807_1700 ESP_018875_1700 (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 | -9.82 | 283. | -6.2 | 16.99 | 60.3 | 58.1 |
| Sinuous Troughs and Ridges near the Sirenum Fossae: ESP_017784_1425 ESP_026276_1425 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 193. | 11.4 | -12.5 | 78.5 | 77.9 |
| 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 |
| 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 |
| Exposure of Polar Layered Deposits: ESP_017954_2720 ESP_018111_2720 (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 | 88.19 | 114. | -9.6 | -16.2 | 63.9 | 65.3 |
| Light-Toned Outcrops in Noctis Region: ESP_017979_1715 ESP_018401_1715 (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 | -8.26 | 267. | -7.1 | -21.7 | 59.6 | 60.6 |
| 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 |
| 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 Deposits in Crater in Western Arabia Terra: ESP_017936_1890 ESP_060489_1890 (Interval in Earth days: 3315) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.810 | -0.9 | 0.22 | -9.82 | 49.5 | 41.2 |
| Mounds and Polygonal Features in Crater: ESP_018078_2445 ESP_018210_2445 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 64.31 | 70.3 | 10.5 | -7.11 | 48.1 | 50.0 |
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