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.
| Rayed Crater West of Granicus Valles: ESP_017048_2040 ESP_017193_2040 (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 | 23.93 | 122. | -7.9 | 4.286 | 42.4 | 41.7 |
| Well-Preserved 15-Kilometer Impact Crater Northwest of Hellas Planitia: ESP_016958_1550 ESP_017736_1550 (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 | -24.6 | 64.4 | 4.47 | -9.81 | 65.7 | 70.5 |
| Head of Chaos Leading to Channel in Margaritifer Terra: ESP_017093_1690 ESP_017238_1690 (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 | -10.9 | 338. | -10. | 3.305 | 58.3 | 58.3 |
| Central Peak with Tilted Bedrock and Megabreccia: ESP_017159_2230 ESP_017304_2230 (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 | 42.62 | 328. | -4.5 | 4.976 | 42.1 | 41.2 |
| Possible Cone Field in Phlegra Dorsa: ESP_017178_2065 ESP_017679_2065 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.35 | 172. | -7.6 | 8.46 | 42.3 | 42.0 |
| Rocky Hill: ESP_016922_1615 ESP_017423_1615 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.5 | 326. | 5.41 | 22.56 | 61.0 | 63.1 |
| Distal Edge of Flow from Galaxias Fossae: ESP_017179_2175 ESP_017245_2175 (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 | 37.16 | 142. | 6.93 | -10.3 | 40.5 | 42.0 |
| Central Structure and Layered Bedrock in 25-Kilometer Diameter Crater: ESP_017002_1535 ESP_017147_1535 (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 | -26.0 | 303. | -3.1 | 10.15 | 67.4 | 67.7 |
| Intersecting Graben in Ulysses Fossae: ESP_017268_1915 ESP_017413_1915 (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 | 11.38 | 237. | -11. | 3.258 | 47.2 | 46.7 |
| Well-Preserved Mid-Latitude Crater: ESP_016981_2210 ESP_017482_2210 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.75 | 149. | -6.3 | 6.555 | 42.1 | 40.9 |
Page 699 of 896 (8,955 images) | |||||