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.
Patchy South Polar Residual Cap in Summertime: ESP_023807_0885 ESP_023713_0915 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.6 | 46.0 | 20.6 | 16.86 | 87.1 | 84.8 |
Recurring Slope Linea Formation in a Well-Preserved Crater: ESP_023586_1425 ESP_024008_1425 (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 | -37.0 | 192. | -3.1 | -14.6 | 42.7 | 50.0 |
Possible Landing Site in Mounds in Central Chryse Region: ESP_023739_2065 ESP_024016_2065 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.28 | 326. | 2.40 | -20.8 | 43.6 | 42.9 |
Tilted Layered Feature among Mesas in Southwest Utopia Planitia: ESP_023603_2175 ESP_024315_2175 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.34 | 77.9 | 0 | 19.54 | 52.9 | 43.8 |
Basal Exposure of South Polar Layered Deposits: ESP_023773_1025 ESP_023615_1025 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -77.2 | 129. | 25.3 | 8.468 | 75.0 | 73.1 |
Dark Lanes in South Polar Residual Cap: ESP_023543_0905 ESP_023531_0905 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.2 | 340. | 26.5 | 25.47 | 81.3 | 81.5 |
Well-Preserved 6-Kilometer Impact Crater: ESP_023828_1820 ESP_031819_1820 (Interval in Earth days: 622) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.091 | 59.3 | 4.49 | -6.67 | 33.0 | 37.8 |
Exposure of South Polar Layered Deposits: ESP_023795_0925 ESP_023691_0925 (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 | -87.4 | 279. | 18.1 | 2.542 | 84.6 | 84.6 |
Possible Hematite and Kieserite in Capri Chasma: ESP_023753_1660 ESP_024320_1660 (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 | -13.8 | 309. | -4.7 | 8.069 | 34.3 | 39.8 |
Small Floral-Shaped Volcano on a Cerberus Fossa: ESP_023811_1880 ESP_024378_1880 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.076 | 162. | 7.71 | 21.56 | 34.0 | 33.7 |
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