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.
| Two Craters along Floor and Wall of Mamers Valles: ESP_033851_2180 ESP_033917_2180 (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 | 37.79 | 15.9 | 9.04 | -7.19 | 41.2 | 42.3 |
| Possible Terraced Crater in Arcadia Planitia: ESP_033739_2290 ESP_034293_2290 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.78 | 192. | -1.3 | -28.2 | 47.4 | 46.8 |
| Shallow Crater with Cross-Cutting Valley: ESP_033880_2200 ESP_034882_2200 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.46 | 305. | -4.8 | 23.57 | 42.8 | 39.0 |
| Deposits in Crater Depression: ESP_033823_2065 ESP_033968_2065 (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 | 26.15 | 62.4 | 5.12 | 19.57 | 38.9 | 37.8 |
| Sinuous Ridges in Aeolis Region: ESP_033820_1735 ESP_034176_1735 (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 | -6.31 | 149. | -0.9 | 14.15 | 46.2 | 49.0 |
| Marte Vallis Lava: ESP_033911_1920 ESP_034267_1920 (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 | 12.03 | 182. | 1.44 | 16.81 | 40.3 | 41.3 |
| Pit Crater on Pavonis Mons: ESP_033935_1805 ESP_041900_1805 (Interval in Earth days: 621) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.323 | 249. | -7.8 | -22.7 | 44.9 | 39.1 |
| Layering in Gorgonum Chaos: ESP_033911_1430 ESP_042443_1430 (Interval in Earth days: 665) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.5 | 188. | -2.9 | -21.5 | 66.6 | 63.7 |
| Dry Cataract in Mangala Valles: ESP_033976_1635 ESP_034609_1635 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.1 | 210. | 8.84 | -15.1 | 52.9 | 60.9 |
| Well-Preserved Impact Crater in Tyrrhena Terra: ESP_033822_1685 ESP_034099_1685 (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 | -11.5 | 95.0 | -0.3 | -25.1 | 49.0 | 53.9 |
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