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.
Arandas Crater in Northern Plains: PSP_010407_2230 ESP_019123_2230 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.43 | 345. | 0 | 17.14 | 52.3 | 48.4 |
Crater in Icaria Fossae Region with Intersecting Graben: ESP_011440_1335 ESP_011941_1335 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.9 | 234. | -5.1 | 15.24 | 68.4 | 59.6 |
Central Uplift of an Impact Crater: PSP_010745_1465 ESP_028006_1465 (Interval in Earth days: 1345) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.2 | 126. | 5.23 | -17.2 | 69.4 | 71.8 |
Persbo Crater: PSP_010836_1885 ESP_081663_1885 (Interval in Earth days: 5519) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.470 | 156. | 1.88 | 19.92 | 54.9 | 55.7 |
Well-Preserved Unnamed Crater in Acidalia Planitia: PSP_010579_2170 ESP_016104_2170 (Interval in Earth days: 431) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.66 | 329. | 4.65 | 19.26 | 52.8 | 40.8 |
Light-Toned Layering in Ladon Valles: PSP_010632_1595 ESP_028394_1595 (Interval in Earth days: 1384) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.5 | 330. | 3.21 | 13.98 | 64.0 | 60.3 |
Cone at the Source of Athabasca Valles: PSP_010770_1905 ESP_011403_1905 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.15 | 157. | 16.7 | -7.00 | 53.1 | 58.4 |
Very Recent Small Crater: PSP_010772_2145 ESP_045136_2145 (Interval in Earth days: 2678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.38 | 100. | 4.13 | -8.37 | 54.7 | 42.8 |
Flow Feature in Southern Utopia Planitia: ESP_011497_1965 ESP_064454_1965 (Interval in Earth days: 4126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.22 | 110. | -4.3 | -24.5 | 59.6 | 61.7 |
Possible MSL Landing Site Mawrth Vallis: PSP_010816_2040 PSP_010882_2040 (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 | 23.95 | 340. | 3.22 | -17.0 | 54.1 | 56.5 |
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