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.
| Landslide Facing North Near Aeolis Mensae: ESP_060286_1735 ESP_063187_1735 (Interval in Earth days: 227) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.58 | 141. | 4.41 | 16.49 | 44.6 | 56.4 |
| Cataract and Grooves in Kasei Valles: ESP_060320_2030 ESP_059964_2030 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.75 | 289. | 6.80 | -8.25 | 36.9 | 37.5 |
| Sinuous Gullies and Arcuate Ridges: ESP_060214_1355 ESP_060280_1355 (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 | -44.1 | 311. | 8.88 | -7.81 | 68.5 | 70.4 |
| Chaotic Terrain Near Ravi Vallis: ESP_060451_1790 ESP_061018_1790 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.98 | 316. | 6.53 | 26.02 | 43.5 | 47.1 |
| Candidate Recent Impact Site: ESP_060062_1840 ESP_060128_1840 (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 | 3.862 | 135. | -0.6 | -21.4 | 38.3 | 40.6 |
| North Flank of Ceti Mensa: ESP_060083_1745 ESP_053832_1745 (Interval in Earth days: 487) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.68 | 284. | -14. | 7.558 | 43.1 | 54.7 |
| Northwestern Rim of Roddy Crater: ESP_060029_1585 ESP_059963_1585 (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 | -21.3 | 320. | -10. | 11.28 | 50.6 | 48.3 |
| Dunes and Steep Slopes in Coprates Chasma: ESP_060188_1660 ESP_060333_1660 (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 | -13.7 | 298. | -3.5 | 16.22 | 47.8 | 48.4 |
| Tilted Layers in Electris Region: ESP_059955_1435 ESP_060232_1435 (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 | -36.0 | 181. | 7.57 | -13.5 | 58.5 | 63.9 |
| Apollinaris Sulci Ancient Dunes: ESP_060166_1675 ESP_060443_1675 (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 | -12.5 | 177. | 6.46 | -16.4 | 46.1 | 51.1 |
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