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.
| Gully Monitoring and Topography: ESP_067155_1415 ESP_074132_1415 (Interval in Earth days: 543) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 195. | 5.52 | 26.12 | 41.5 | 49.6 |
| Mass Wasting Features on Crater Wall: ESP_067151_2105 ESP_067494_2105 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.28 | 296. | -5.4 | 7.379 | 58.8 | 53.9 |
| Dipping Layers in Crater in Southern Mid-Latitudes: ESP_067118_1415 ESP_067659_1415 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 125. | 2.08 | -7.47 | 41.5 | 48.5 |
| Gully Stratigraphy with Glacial Deposits: ESP_066970_1395 ESP_074079_1395 (Interval in Earth days: 554) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.0 | 204. | -6.1 | 6.702 | 41.7 | 52.2 |
| Gullies Emanating from Lobate Flow: ESP_067296_1315 ESP_058856_1315 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.0 | 309. | 9.71 | -12.4 | 47.6 | 50.0 |
| Surface Features in Hellas Planitia: ESP_067279_1480 ESP_067345_1480 (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 | -31.4 | 50.9 | 6.46 | -2.66 | 40.1 | 41.3 |
| Spider Terrain: ESP_066936_0930 ESP_066963_0930 (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 | -86.8 | 86.2 | 14.5 | 4.628 | 69.8 | 71.1 |
| Auqakuh Vallis: ESP_067054_2125 ESP_084409_2125 (Interval in Earth days: 1352) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.38 | 61.9 | 5.60 | -11.2 | 60.8 | 64.2 |
| Layering in Rutherford Crater: ESP_066938_1990 ESP_067070_1990 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.94 | 349. | -0.3 | -20.9 | 53.4 | 53.2 |
| Lobate Apron in Phlegra Montes: ESP_067169_2165 ESP_067301_2165 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.01 | 164. | 0.39 | -14.9 | 62.3 | 61.5 |
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