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.
| Crater in Arabia Terra: ESP_087747_2200 ESP_087681_2200 (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 | 39.57 | 7.75 | -7.8 | 6.691 | 43.3 | 42.0 |
| USGS Dune Database Entry Number 1384-341: ESP_087637_1455 ESP_087703_1455 (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 | -34.2 | 138. | 8.46 | -9.95 | 74.4 | 75.9 |
| Layering in Inverted Crater: ESP_087833_1725 ESP_088123_1725 (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 | -7.44 | 186. | -19. | -2.53 | 59.3 | 59.4 |
| North-Pole-Facing Deposit in Crater: ESP_087778_2285 ESP_088068_2285 (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 | 48.34 | 240. | -10. | 2.734 | 44.8 | 43.5 |
| Inverted Drainage Network Deep in Central Valles Marineris: ESP_087816_1705 ESP_088027_1705 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.41 | 289. | 6.89 | -9.49 | 58.7 | 60.7 |
| Ares Vallis: ESP_087933_1945 ESP_088645_1945 (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 | 14.31 | 331. | 6.80 | -6.85 | 46.7 | 49.7 |
| Crater with Evidence of Glacial Erosion: ESP_087913_2160 ESP_088124_2160 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.79 | 156. | -6.9 | -20.2 | 43.2 | 44.7 |
| 4-Kilometer Diameter Rayed Crater: ESP_087802_1915 ESP_088448_1915 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.13 | 309. | 0.34 | 12.37 | 48.0 | 49.1 |
| Layering in Heavily Cratered Lucus Planum Terrain: ESP_087820_1755 ESP_088110_1755 (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 | -4.46 | 179. | 0.91 | 19.03 | 56.1 | 56.1 |
| Channels Going Into Echus Chasma: ESP_087724_1850 ESP_088792_1850 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.863 | 278. | 5.37 | -4.74 | 50.2 | 53.9 |
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