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.
| Crater with Viscous Flows and a Channel: ESP_025970_2235 ESP_025904_2235 (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 | 42.90 | 257. | -8.9 | 7.02 | 41.4 | 40.1 |
| Light-Toned Material along Coprates Chasma Wallrock and Plateau: ESP_025929_1645 ESP_026430_1645 (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 | -15.5 | 303. | -6.5 | 17.74 | 60.0 | 61.1 |
| Dark Slope Streak Extending to Channel Floor: ESP_026064_2045 ESP_026697_2045 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.17 | 212. | 0 | -15.4 | 41.0 | 44.0 |
| Newton Crater Valleys and Alluvial Fans: ESP_026012_1410 ESP_026078_1410 (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 | -38.7 | 199. | 4.09 | -15.0 | 76.7 | 78.1 |
| Small Fresh Crater on Northern Plains: ESP_026076_2320 ESP_026419_2320 (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 | 51.66 | 236. | 24.6 | -3.11 | 40.7 | 42.9 |
| Streamlined Forms in Elysium Planitia: ESP_025802_1960 ESP_026435_1960 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.72 | 165. | 7.87 | -11.1 | 41.7 | 45.6 |
| Well-Preserved Impact Crater on Floor of Coprates Chasma: ESP_025982_1675 ESP_025626_1675 (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 | -12.3 | 294. | 14.8 | 0 | 56.9 | 55.1 |
| Mound with Linear Depression at Summit in Center of Crater: ESP_026042_2020 ESP_028574_2020 (Interval in Earth days: 198) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.91 | 93.1 | 2.80 | -9.54 | 41.2 | 53.6 |
| Tharsis Region Lava Flow: ESP_026010_1940 ESP_025733_1940 (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 | 13.65 | 250. | -22. | 2.608 | 45.8 | 42.5 |
| Layered Flow Ejecta: ESP_026109_1575 ESP_026531_1575 (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 | -22.1 | 70.4 | -8.4 | -20.1 | 65.8 | 68.2 |
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