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.
Layers in Depression Walls Revealing Structure of Crater Ice Fill: ESP_087798_2270 ESP_087719_2270 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.69 | 54.0 | -5.1 | -28.4 | 43.9 | 46.3 |
Overlapping Landslides in Crater in Margaritifer Terra: ESP_087603_1925 ESP_087880_1925 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.18 | 338. | 28.7 | 9.699 | 44.3 | 47.2 |
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 |
Layering in Western Lucus Planum: ESP_087912_1725 ESP_087978_1725 (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 | -7.58 | 187. | 5.90 | -20.6 | 58.1 | 60.2 |
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 |
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 |
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 |
Terrain East of Schiaparelli Crater: ESP_087773_1770 ESP_088485_1770 (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 | -2.90 | 22.3 | 4.38 | -6.57 | 54.7 | 57.8 |
Athabasca Valles: ESP_087834_1895 ESP_088401_1895 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.534 | 156. | -2.1 | -25.3 | 49.0 | 52.7 |
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 |
Page 10 of 857 (8,562 images) |