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.
| East Coprates Chasma Dune Fields and Wall Rock: ESP_025164_1655 ESP_025731_1655 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 306. | 10.3 | 21.59 | 50.8 | 55.8 |
| Beautiful Butterfly Crater (HiWish Granted Again): ESP_029854_1890 ESP_029999_1890 (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 | 9.002 | 69.0 | -19. | -0.82 | 58.7 | 57.3 |
| Banded Bedrock in Terra Sabaea: ESP_030184_1585 ESP_030606_1585 (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 | -21.2 | 62.0 | -8.2 | -24.9 | 47.6 | 43.9 |
| Noachis Region Dune Changes: ESP_030080_1245 ESP_030014_1245 (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 | -55.0 | 26.8 | -3.4 | 13.05 | 54.0 | 53.9 |
| Possible Phyllosilicate Deposit in Valles Marineris : ESP_029569_1675 ESP_056720_1675 (Interval in Earth days: 2116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 290. | 5.53 | -4.17 | 52.7 | 46.2 |
| Possible Fan in Crater : ESP_029490_1565 ESP_029912_1565 (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 | -23.3 | 288. | 3.81 | -10.5 | 53.9 | 50.7 |
| Layered Material in Melas Chasma : ESP_029411_1690 ESP_055599_1690 (Interval in Earth days: 2040) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.6 | 284. | -1.8 | 24.60 | 54.1 | 51.0 |
| Interesting Young Flow Features in Nereidum Montes : ESP_029634_1430 ESP_041001_1430 (Interval in Earth days: 886) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.5 | 319. | 4.54 | -22.6 | 54.6 | 42.3 |
| Lobate Form with Digitate Ridges on Northwest Wall of Nicholson Crater : ESP_029612_1810 ESP_030390_1810 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.731 | 195. | 4.16 | -10.8 | 54.4 | 52.5 |
| Light-Toned Layered Rock Exposure in Holden Crater Secondary Crater : ESP_029515_1590 ESP_030293_1590 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.6 | 325. | 5.81 | -8.64 | 53.2 | 46.4 |
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