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.
| Diverse Lithologies in Central Uplift of Stokes Crater: ESP_019380_2360 ESP_019604_2360 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.59 | 171. | -16. | 10.82 | 58.7 | 59.7 |
| Flow Material in Equatorial Crater: ESP_019267_1720 ESP_024858_1720 (Interval in Earth days: 436) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.05 | 23.2 | -8.4 | -26.9 | 58.1 | 46.5 |
| Crater in Sinus Sabaeus Region: ESP_019386_1700 ESP_020019_1700 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.0 | 13.6 | 3.93 | -10.0 | 57.8 | 57.1 |
| Bedrock in Walls of Well-Preserved Impact Crater in Tartarus Montes: ESP_019222_2055 ESP_019367_2055 (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 | 25.03 | 167. | -7.6 | 5.969 | 49.8 | 49.8 |
| Bedrock in Hydrae Chasma: ESP_019336_1730 ESP_019969_1730 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.75 | 297. | 8.78 | -6.40 | 56.2 | 56.2 |
| Excellent Megabreccia Outcrops along the Walls of Nili Fossae: ESP_019476_2005 ESP_019621_2005 (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 | 20.23 | 73.7 | -7.1 | 8.669 | 51.7 | 51.4 |
| Light-Toned Unit along Coprates Region Ridge: ESP_019468_1670 ESP_019534_1670 (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 | -13.0 | 295. | 5.62 | -17.3 | 58.7 | 60.1 |
| North Polar Residual Cap: ESP_019282_2675 ESP_019257_2675 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.69 | 274. | -8.5 | -21.6 | 73.4 | 73.5 |
| Distal Margins of the Western Ejecta of Corinto Crater: ESP_019579_1970 ESP_019935_1970 (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 | 16.91 | 141. | 0.39 | 12.99 | 51.8 | 53.3 |
| Central Uplift in Baldet Crater: ESP_019529_2030 ESP_025120_2030 (Interval in Earth days: 435) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.68 | 65.6 | 1.83 | -17.0 | 51.3 | 39.8 |
Page 643 of 878 (8,772 images) | |||||