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.
| Light-Toned Fan-Like Features in Crater in Chryse Chaos: ESP_013256_1885 ESP_022104_1885 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.534 | 327. | -1.4 | -13.8 | 53.6 | 52.2 |
| Strike Slip Fault in Amazonis Planitia: ESP_012799_1990 ESP_013076_1990 (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 | 18.75 | 203. | 1.92 | -21.6 | 63.2 | 63.0 |
| Gullies Previously Identified in MOC Image: ESP_013849_1080 ESP_013981_1080 (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 | -71.9 | 354. | -7.6 | -22.1 | 56.8 | 59.0 |
| Warrego Valles Headwater Region: ESP_013153_1390 ESP_013298_1390 (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 | -40.6 | 266. | -5.4 | 6.316 | 42.0 | 39.7 |
| Chain of Cones and Craters in Isidis Planitia: ESP_013054_1900 ESP_013199_1900 (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 | 9.766 | 83.1 | -5.1 | 9.582 | 56.5 | 54.2 |
| Basal Exposure of South Polar Layered Deposits: ESP_013145_1070 ESP_013277_1070 (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 | -73.0 | 133. | 0.46 | -14.5 | 55.6 | 56.1 |
| Pits in Hydrae Chasma: ESP_013033_1730 ESP_013745_1730 (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 | -6.83 | 297. | 0 | 14.87 | 47.8 | 38.4 |
| Layered Crater Fill Material: ESP_014017_2085 ESP_022021_2085 (Interval in Earth days: 624) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.99 | 68.5 | 0.69 | 16.01 | 57.5 | 64.7 |
| Gullies in Light-Toned Rock: ESP_012795_1395 ESP_013507_1395 (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 | -40.2 | 319. | 2.74 | 16.59 | 45.9 | 37.2 |
| Exposure of Layers in South Gale Crater with Possible Sulfates: ESP_014186_1745 ESP_020410_1745 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.56 | 138. | 8.10 | -13.1 | 35.2 | 55.9 |
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