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.
| Channel and Stepped Fan in Graben Near Valles Marineris : ESP_045551_1715 ESP_052078_1715 (Interval in Earth days: 509) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.32 | 296. | -5.9 | -23.5 | 54.6 | 53.1 |
| Large Alcove Dunes : ESP_045571_2565 ESP_046375_2565 (Interval in Earth days: 63) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.19 | 95.3 | -7.4 | 13.71 | 63.2 | 74.7 |
| Impact Crater and Ejecta Partially Buried by Lobate Debris Apron : ESP_045640_2210 ESP_050901_2210 (Interval in Earth days: 410) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.60 | 21.0 | -8.8 | 6.271 | 47.8 | 44.7 |
| Possible Exposure of North Polar Layered Deposits : ESP_045576_2710 ESP_045353_2710 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.78 | 139. | -26. | -20.6 | 74.4 | 71.2 |
| Well-Preserved 6-Kilometer Impact Crater : ESP_045601_1590 ESP_044124_1590 (Interval in Earth days: 115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.9 | 12.7 | 1.66 | -13.0 | 60.9 | 65.9 |
| Exposure of North Polar Layered Deposits: ESP_045407_2660 ESP_045485_2660 (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 | 86.16 | 232. | -8.8 | 5.759 | 67.9 | 68.6 |
| Deposits in Noctis Labyrinthus : ESP_045763_1725 ESP_046541_1725 (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 | -7.70 | 266. | 12.7 | 0.053 | 52.6 | 52.2 |
| High-Latitude Exposure of North Polar Layered Deposits : ESP_045443_2690 ESP_045547_2690 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.77 | 9.66 | -26. | -21.6 | 71.3 | 72.1 |
| Landforms in Utopia Planitia : ESP_045756_2135 ESP_052217_2135 (Interval in Earth days: 504) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.18 | 94.1 | -2.9 | 6.466 | 47.0 | 37.8 |
| Crater with Persistent Ice : ESP_045503_2540 ESP_045160_2540 (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 | 73.88 | 152. | -3.1 | 6.7 | 60.7 | 56.4 |
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