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.
| Chaotic Terrain in Xanthe Terra: ESP_066913_1780 ESP_075011_1780 (Interval in Earth days: 631) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.09 | 315. | -8.7 | -22.8 | 42.7 | 49.2 |
| 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 |
| 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 |
| Feature on South Polar Layered Deposits: ESP_066960_0920 ESP_067143_0920 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 194. | 11.8 | 22.61 | 71.9 | 73.0 |
| 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 Monitoring: ESP_067152_1310 ESP_067429_1310 (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 | -48.5 | 280. | -5.5 | 12.24 | 47.2 | 49.7 |
| Layering in Arabia Terra: ESP_067228_1820 ESP_074205_1820 (Interval in Earth days: 544) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.134 | -0.7 | -6.5 | 5.414 | 42.1 | 56.2 |
| Fans and Polygons: ESP_067026_0925 ESP_066959_0925 (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 | -87.2 | 167. | 8.81 | 21.59 | 72.0 | 69.8 |
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