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.
| Partially-Buried Pre-Existing Crater: PSP_007524_1400 ESP_016108_1400 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 234. | -1.4 | -18.6 | 70.0 | 67.6 |
| Dark Dune-Like Forms in Southern Melas Chasma: PSP_007522_1685 ESP_025666_1685 (Interval in Earth days: 1414) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 284. | 0.94 | -27.7 | 51.1 | 56.6 |
| Central Peak Region of Canso Crater: PSP_007139_2015 ESP_085442_2015 (Interval in Earth days: 6101) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.34 | 299. | -1.5 | -10.2 | 39.3 | 44.2 |
| Layering in East Coprates Chasma Wall: PSP_007864_1655 PSP_007508_1655 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 307. | -8.1 | 4.599 | 57.2 | 52.4 |
| Rayed Crater with Central Peak at Acidalia Planitia-Arabia Terra Boundary: PSP_007123_2250 ESP_023803_2250 (Interval in Earth days: 1300) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.71 | 12.7 | -0.0 | 26.95 | 46.9 | 54.3 |
| Diverse Features in Utopia Region: PSP_007951_2220 PSP_008162_2220 (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 | 41.58 | 82.8 | 6.93 | -5.86 | 41.7 | 42.5 |
| Recent 6-Kilometer Diameter Crater in Acidalia Planitia: PSP_007982_2125 ESP_015933_2125 (Interval in Earth days: 620) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.28 | 318. | -3.1 | 18.34 | 41.4 | 40.0 |
| Rocky Central Uplift of 80-Kilometer Diameter Crater: PSP_007978_2005 ESP_024487_2005 (Interval in Earth days: 1286) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.18 | 69.4 | 0 | -26.2 | 42.1 | 39.4 |
| Fresh Double Layer Ejecta Crater in Northern Plains: PSP_007736_2345 PSP_008303_2345 (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 | 54.37 | 190. | 8.23 | -7.73 | 47.0 | 45.9 |
| Area Near Summit of Gale Crater Mound: PSP_008002_1750 PSP_009927_1750 (Interval in Earth days: 151) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.85 | 137. | -5.8 | -22.8 | 52.8 | 59.9 |
Page 800 of 878 (8,772 images) | |||||