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.
Pit and Channel on Southwestern Pavonis Mons: PSP_009923_1785 PSP_010213_1785 (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 | -1.67 | 246. | -21. | 14.06 | 58.1 | 55.7 |
Look for Change Due to Mass Wasting on Scarps of Different Slopes: PSP_009408_2640 PSP_009882_2640 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.00 | 230. | 0.72 | 16.89 | 60.3 | 62.9 |
High-Latitude Exposure of North Polar Layered Deposits: PSP_010100_2675 PSP_010457_2675 (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 | 87.29 | 32.0 | -5.8 | -15.5 | 68.3 | 73.1 |
Distributaries From Athabasca Valles: PSP_009768_1880 PSP_010045_1880 (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 | 7.721 | 154. | 7.98 | -19.7 | 51.6 | 54.3 |
Unconformities in North Polar Layered Deposits: PSP_010124_2650 PSP_010242_2650 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.81 | 128. | -7.7 | 7.364 | 67.0 | 67.7 |
Fresh Crater Cluster Formed between June 4 2008 and August 10 2008: PSP_010189_2265 PSP_010334_2265 (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 | 46.33 | 176. | -6.2 | 4.534 | 51.2 | 51.8 |
Well-Preserved Crater with Central Peak: PSP_009367_1590 ESP_035357_1590 (Interval in Earth days: 2025) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.6 | 306. | -5.0 | 9.569 | 68.4 | 66.5 |
Clays Exposed in Channels along West Ladon Valles: PSP_010342_1600 ESP_034552_1600 (Interval in Earth days: 1886) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.6 | 327. | 0.85 | -19.2 | 65.0 | 63.0 |
Mamers Valles: PSP_009773_2165 ESP_053789_2165 (Interval in Earth days: 3429) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.13 | 14.3 | 5.21 | -4.42 | 45.5 | 42.7 |
High-Latitude Exposure of North Polar Layered Deposits: PSP_009301_2720 PSP_009528_2680 (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 | 88.07 | 204. | -7.9 | -21.1 | 63.9 | 64.7 |
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