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.
| Gale Crater - Potential MSL Landing Site: PSP_010639_1755 PSP_010573_1755 (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 | -4.49 | 137. | -2.2 | 21.20 | 57.9 | 56.0 |
| 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 |
| Possible Inverted Meanders in Filled Channel West of Ladon Valles: ESP_011476_1600 ESP_014100_1600 (Interval in Earth days: 205) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.8 | 327. | -4.0 | 9.389 | 59.7 | 33.0 |
| 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 |
| Phyllosilicate Ring in Terra Sirenum: PSP_010901_1510 ESP_055194_1510 (Interval in Earth days: 3452) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.9 | 187. | 0.35 | -23.2 | 66.4 | 62.6 |
| Light-Toned Bedrock Exposed in Walls and Central Peak of Crater: ESP_011314_1585 ESP_011591_1585 (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 | -21.4 | 70.0 | 5.84 | -21.8 | 60.4 | 60.7 |
| Central Region of an Impact Crater: PSP_010812_1665 ESP_027730_1665 (Interval in Earth days: 1319) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 94.9 | 0.22 | 14.92 | 60.5 | 59.2 |
| Stratigraphy of Primary Mesa in Terby Crater: PSP_010826_1525 ESP_016272_1525 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 74.2 | 4.13 | -10.0 | 65.9 | 60.7 |
| Mounds on Kashira Crater Floor: ESP_011370_1525 ESP_029053_1525 (Interval in Earth days: 1378) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 341. | 8.46 | -10.0 | 61.4 | 59.8 |
| Shalbatana Vallis: PSP_010461_1845 ESP_016619_1845 (Interval in Earth days: 480) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.397 | 315. | 0 | 0 | 54.7 | 45.8 |
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