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.
Alluvial Fans and Hanging Valley Morphology in Kasei Valles: ESP_024215_2030 ESP_024637_2030 (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 | 22.69 | 291. | 8.75 | -2.72 | 37.8 | 37.9 |
Mantle Removal around Gully Fan: ESP_024027_1345 ESP_024304_1345 (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 | -45.4 | 33.9 | -5.9 | -21.5 | 55.7 | 61.3 |
Proctor Crater Dune Changes: ESP_024291_1320 ESP_024370_1320 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.6 | 30.3 | -29. | -0.98 | 63.3 | 62.9 |
Harmakhis Vallis Terrain Sample: ESP_024249_1405 ESP_024394_1405 (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 | -39.2 | 92.0 | -1.1 | 16.31 | 54.7 | 56.2 |
Candor Chasma Dune Changes: ESP_024255_1750 ESP_024110_1750 (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 | -4.79 | 283. | 0.86 | -19.4 | 36.3 | 36.6 |
Gullied Crater Wall in Southeastern Terra Cimmeria: ESP_024286_1330 ESP_024576_1330 (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 | -46.4 | 163. | -3.9 | 19.77 | 60.7 | 64.3 |
Crater Rim with Possible Columnar Jointing: ESP_024288_1945 ESP_024710_1945 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.52 | 98.3 | 21.7 | 6.703 | 34.1 | 36.4 |
Possible Future Landing Site at Edge of Libya Montes: ESP_024038_1835 ESP_023405_1835 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.516 | 86 | 5.65 | 27.23 | 33.6 | 32.4 |
MSL Rover Landing Site in Gale Crater: ESP_024234_1755 ESP_024300_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 | -4.64 | 137. | -5.2 | -24.4 | 36.6 | 38.8 |
Possible Bedform Changes in Medusae Fossae: ESP_024047_1895 ESP_024113_1895 (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 | 9.508 | 197. | 25.0 | 5.939 | 32.7 | 34.4 |
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