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.
| Cones within Acidalia Planitia: ESP_069485_2260 ESP_069841_2260 (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 | 45.48 | 341. | -7.4 | 13.52 | 49.9 | 47.3 |
| Fresh Small Impact Crater: ESP_069405_1790 ESP_069893_1790 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.77 | 9.55 | 4.18 | -5.40 | 54.5 | 58.6 |
| 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 |
| Landforms near Phoenix Landing Site: ESP_069304_2480 ESP_063473_2480 (Interval in Earth days: 454) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.96 | 233. | 0.40 | 25.60 | 58.5 | 61.0 |
| Crater in Arabia Terra: ESP_069537_2190 ESP_070170_2190 (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 | 38.81 | 1.59 | 5.54 | -8.03 | 47.7 | 47.8 |
| 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 |
| Iani Chaos: ESP_069406_1780 ESP_069340_1780 (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 | -2.15 | 343. | -7.7 | 7.5 | 56.0 | 54.3 |
| Fractured Crater: ESP_069225_2485 ESP_063434_2485 (Interval in Earth days: 451) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.19 | 231. | -4.1 | -20.0 | 59.6 | 64.2 |
| 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 |
| 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 |
Page 180 of 881 (8,805 images) | |||||