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.
| Fresh Impact Crater with Dark Ejecta Pattern near Schroeter Crater: ESP_069377_1805 ESP_070155_1805 (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 | 0.625 | 53.6 | 3.51 | 17.75 | 53.7 | 56.9 |
| Layered Positive Relief in Association with Osuga Valles Depression: ESP_069420_1655 ESP_069354_1655 (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 | -14.4 | 322. | -8.9 | 6.438 | 62.4 | 60.6 |
| Crater and Athabasca Valles Flow: ESP_069558_1865 ESP_069624_1865 (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 | 6.546 | 152. | 8.03 | -6.63 | 52.6 | 54.2 |
| Enigmatic Channel in Syrtis Major Region: ESP_069495_1955 ESP_069706_1955 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.39 | 74.4 | -29. | -13.2 | 52.5 | 52.3 |
| Layering in Wall of Orson Welles Crater: ESP_069407_1795 ESP_070330_1795 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.65 | 315. | 3.10 | 21.96 | 54.6 | 57.4 |
| Light-Toned Layered Deposits in Ladon Valles Basin: ESP_069301_1595 ESP_069367_1595 (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 | -20.2 | 329. | 7.95 | -6.97 | 63.1 | 64.9 |
| Flow Features inside Eastern Floor of Crater South of Burton Crater: ESP_069332_1640 ESP_069675_1640 (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 | -15.7 | 203. | 2.59 | -8.01 | 61.3 | 65.8 |
| A Second Look at the Zhurong Lander: ESP_069731_2055 ESP_069665_2055 (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 | 25.10 | 109. | -5.1 | 10.30 | 49.5 | 47.9 |
| Stratigraphy Exposed in Walls of Hephaestus Fossae: ESP_069071_2020 ESP_063847_2020 (Interval in Earth days: 407) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.82 | 122. | 3.59 | -29.3 | 46.4 | 57.5 |
| Layered Deposits in Jiji Crater: ESP_069102_1890 ESP_069234_1890 (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 | 8.759 | 358. | -1.7 | -29.0 | 48.9 | 52.4 |
Page 195 of 896 (8,955 images) | |||||