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.
| Lineated Valley Fill in Coloe Fossae: PSP_008743_2155 PSP_009033_2155 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.34 | 57.0 | 1.58 | 10.94 | 42.0 | 41.8 |
| Lobate Debris Apron with Ridge-Like Structures in Tempe Terra: PSP_008563_2320 PSP_008774_2320 (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 | 51.77 | 288. | 6.33 | -7.60 | 43.4 | 44.6 |
| Relatively Deeply Eroded Portion of Marte Vallis: PSP_008567_1985 PSP_008923_1985 (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 | 18.26 | 185. | 6.87 | -12.2 | 44.4 | 47.1 |
| Bedrock Exposed in Crater Wall in Acidalia Region: PSP_009036_2250 ESP_062850_2250 (Interval in Earth days: 4193) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.59 | 335. | -3.5 | 15.73 | 43.4 | 45.5 |
| Near the Head of Lethe Vallis: PSP_009056_1840 PSP_009900_1840 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.802 | 153. | 6.66 | -22.9 | 52.4 | 55.9 |
| Exposure of Polar Layered Deposits Not Well Observed by Previous Missions: PSP_009039_2680 PSP_009133_2680 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.00 | 169. | -8.0 | -15.3 | 63.1 | 63.0 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009187_2680 ESP_018221_2680 (Interval in Earth days: 704) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.92 | 95.3 | -6.5 | -14.0 | 63.1 | 63.7 |
| Northern Hemisphere Polygons and Seasonal Spots: PSP_009159_2650 PSP_009753_2650 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.98 | 194. | -8.3 | -22.1 | 60.6 | 64.5 |
| Very Fresh Small Crater in Arabia Region: PSP_009206_1920 ESP_062941_1915 (Interval in Earth days: 4187) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.71 | 17.8 | 3.16 | -6.38 | 49.2 | 50.5 |
| Concentric Ridges Near Alcoves Northwest of Oudemans Crater: PSP_008986_1715 PSP_009408_1715 (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 | -8.27 | 266. | 8.18 | -9.64 | 59.2 | 60.9 |
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