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.
| Streamlined Landforms in THEMIS Image V27359007: ESP_032745_1415 ESP_032811_1415 (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 | -38.3 | 341. | 19.2 | 0.849 | 47.9 | 50.1 |
| Gullies in Pit Wall: ESP_032652_1300 ESP_024226_1300 (Interval in Earth days: 656) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.8 | 3.92 | 1.38 | -19.6 | 55.6 | 63.1 |
| Layered Materials on Northeast Hellas Region Rim: ESP_032636_1525 ESP_032781_1525 (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 | -27.3 | 78.1 | -7.4 | 7.913 | 41.3 | 42.4 |
| Fractured Ground in Arabia Terra: ESP_032770_2155 ESP_032915_2155 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.15 | 11.8 | -6.6 | 4.794 | 48.1 | 45.9 |
| Valley Headwalls: ESP_032743_2205 ESP_032888_2205 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.04 | 26.1 | 11.6 | 21.84 | 50.5 | 48.2 |
| Light-Toned Stratified Materials in Melas Chasma: ESP_032747_1690 ESP_033169_1690 (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 | -10.5 | 285. | -2.6 | -24.4 | 35.6 | 42.1 |
| Very Well-Preserved Crater in Ares Vallis: ESP_032521_1955 ESP_032943_1955 (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 | 15.35 | 331. | 8.89 | -7.24 | 37.8 | 37.5 |
| Large Dated Impact Crater: ESP_032881_1855 ESP_032736_1855 (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 | 5.457 | 224. | 2.57 | -13.9 | 34.8 | 35.7 |
| Bright Dunes South of Echus Chasma: ESP_032734_1780 ESP_058804_1780 (Interval in Earth days: 2031) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.00 | 279. | -8.6 | 20.37 | 34.8 | 29.5 |
| USGS Dune Database Entry Number 0045-031: ESP_032744_1830 ESP_032955_1830 (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 | 3.103 | 4.57 | 6.42 | -3.11 | 33.9 | 35.5 |
Page 499 of 878 (8,772 images) | |||||