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.
| Ares Vallis: ESP_066055_1955 ESP_065923_1955 (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 | 15.47 | 328. | -5.1 | 20.08 | 60.9 | 60.2 |
| Valley Cutting Ejecta of Crater and Associated Sinuous Ridge: ESP_065902_1685 ESP_065968_1685 (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 | -11.3 | 185. | 7.46 | -6.99 | 47.9 | 48.2 |
| Hydrated Sulfate-Rich Terrain in Aram Chaos: ESP_066081_1830 ESP_092930_1830 (Interval in Earth days: 2092) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.992 | 339. | -0.1 | -20.4 | 53.1 | 48.0 |
| Layering in Western Arabia Terra: ESP_065909_1895 ESP_065975_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 | 9.623 | 352. | 6.43 | -7.49 | 57.8 | 58.2 |
| Layers: ESP_065906_1520 ESP_065207_1520 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.8 | 78.5 | 8.66 | -11.8 | 44.1 | 53.9 |
| Gully Monitoring and Topography: ESP_065744_1410 ESP_065876_1410 (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 | -38.6 | 181. | 2.17 | -22.2 | 46.5 | 46.8 |
| Well-Preserved Impact Crater: ESP_065749_1375 ESP_065195_1375 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.9 | 46.3 | -2.8 | 7.31 | 47.3 | 54.2 |
| Contact between Medusae Fossae Formation and Apollinaris Mons Flank: ESP_065942_1725 ESP_066008_1725 (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 | -7.30 | 173. | 8.42 | -5.76 | 48.9 | 49.3 |
| Layers in Crater: ESP_065855_1820 ESP_065987_1820 (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 | 1.995 | 27.0 | 3.96 | -23.6 | 54.3 | 55.1 |
| Cluster of Small Cones in Baetis Chaos: ESP_065977_1770 ESP_065911_1770 (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 | -2.86 | 299. | -7.7 | 6.708 | 51.7 | 51.3 |
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