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.
| Exposure of Layers in South Gale Crater with Possible Sulfates: ESP_014186_1745 ESP_020410_1745 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.56 | 138. | 8.10 | -13.1 | 35.2 | 55.9 |
| Western Half of Very Well-Preserved Gullied Crater: ESP_012807_1505 ESP_012952_1505 (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 | -29.4 | 351. | -5.9 | 9.919 | 45.8 | 42.6 |
| Ares Vallis Wall and Floor Exposures: ESP_013216_1870 ESP_022143_1870 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.694 | 340. | -2.5 | 20.39 | 53.0 | 48.5 |
| Gullies Oriented around Large Obstacle in MOC Image E1002766: ESP_014132_1425 ESP_020791_1425 (Interval in Earth days: 519) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 178. | -8.6 | 14.15 | 38.0 | 54.6 |
| Stratigraphic Relations in THEMIS Image V11134006 in Sinus Meridiani: ESP_013703_1800 ESP_021984_1800 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.14 | 2.99 | 25.0 | 10.04 | 41.4 | 46.9 |
| Ejecta Falling Into Earlier Large Crater: ESP_013346_1940 ESP_013768_1940 (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 | 13.86 | 29.4 | 6.71 | -7.95 | 55.5 | 51.3 |
| Gullies Incised on Crater Wall: PSP_001578_1425 PSP_002066_1425 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.9 | 206. | -3.7 | 13.99 | 73.9 | 68.4 |
| Interesting Crater in Meridiani Planum: PSP_001348_1770 PSP_001678_1770 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.06 | 356. | -4.0 | -27.6 | 56.4 | 58.1 |
| Ridges and Layered Deposits Near Capri Mensa: PSP_001376_1675 PSP_001574_1675 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.2 | 314. | -4.1 | -19.0 | 60.8 | 61.3 |
| Starburst Spider Forms: ESP_014255_0980 ESP_014281_0980 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.7 | 76.0 | 6.80 | 24.45 | 68.6 | 68.0 |
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