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.
| Gullies: ESP_065408_1420 ESP_073546_1420 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.6 | 351. | 6.35 | 29.29 | 50.5 | 57.6 |
| Lava-Filled Crater near Athabasca Valles: ESP_065481_1875 ESP_065969_1875 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.224 | 154. | -0.2 | 16.82 | 59.3 | 55.2 |
| Gullied Slope: ESP_065466_1455 ESP_065809_1455 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.1 | 209. | -3.7 | -19.0 | 50.3 | 47.1 |
| Gullies in Nereidum Montes: ESP_065515_1400 ESP_065937_1400 (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 | -39.4 | 312. | -1.0 | 25.03 | 49.9 | 42.5 |
| Gully Monitoring and Topography: ESP_065335_1415 ESP_065757_1415 (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 | -38.2 | 185. | -5.2 | 15.91 | 52.5 | 45.3 |
| Cones in Utopia Planitia: ESP_065298_2060 ESP_091765_2060 (Interval in Earth days: 2062) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.74 | 105. | 8.28 | -13.3 | 68.1 | 68.9 |
| Layering in Arabia Terra: ESP_065289_1835 ESP_065355_1835 (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 | 3.606 | 355. | -5.9 | -23.2 | 58.8 | 60.0 |
| Streamlined Feature in Marte Vallis: ESP_065203_1910 ESP_066100_1910 (Interval in Earth days: 70) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.90 | 182. | -5.9 | -23.5 | 61.8 | 58.9 |
| Crater: ESP_065200_1470 ESP_065899_1470 (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 | -32.4 | 269. | -7.6 | 12.08 | 53.9 | 43.7 |
| Proximal End of Marte Vallis System: ESP_065190_1875 ESP_074027_1875 (Interval in Earth days: 688) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.361 | 177. | -5.8 | 18.98 | 60.4 | 57.8 |
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