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.
| Flow-Like Features Near Kasei Valles: ESP_043085_2070 ESP_043797_2070 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.95 | 290. | 4.74 | 24.01 | 39.0 | 37.9 |
| Expanded Secondary Craters in Arcadia Planitia: ESP_042784_2355 ESP_044063_2355 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.30 | 224. | -4.8 | 10.36 | 49.4 | 42.4 |
| Concentric Crater Fill: ESP_042931_2315 ESP_043208_2315 (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 | 51.07 | 171. | -3.0 | -19.5 | 46.1 | 45.9 |
| Small Buttes and Dunes in Meridiani Planum: ESP_042951_1820 ESP_043017_1820 (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 | 2.207 | 352. | -4.3 | -26.0 | 45.2 | 47.4 |
| USGS Dune Database Number 0380-426 Changes: ESP_042343_1370 ESP_033811_1370 (Interval in Earth days: 664) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.6 | 38.0 | 0.13 | 15.08 | 65.4 | 68.7 |
| Lineated Valley Floor Material in Terrain North of Arabia Region: ESP_042435_2210 ESP_042725_2210 (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 | 40.95 | 34.6 | 4.68 | 21.72 | 44.2 | 41.0 |
| Oxia Palus Region: ESP_042134_1985 ESP_053962_1985 (Interval in Earth days: 922) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.04 | 335. | 7.47 | -28.4 | 37.8 | 47.7 |
| Daedalia Planum Lava Flows: ESP_042296_1545 ESP_042362_1545 (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 | -25.1 | 236. | 23.7 | 0.587 | 51.3 | 53.7 |
| Ridge in Southern Melas Chasma: ESP_042571_1675 ESP_059028_1675 (Interval in Earth days: 1282) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 286. | 22.2 | -4.42 | 47.2 | 32.7 |
| Aram Chaos Slope Monitoring Site: ESP_042490_1835 ESP_042635_1835 (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 | 3.297 | 339. | -7.2 | 5.79 | 41.7 | 41.7 |
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