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.
| Well-Preserved 3-Kilometer Impact Crater : ESP_049070_1940 ESP_058947_1940 (Interval in Earth days: 769) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.93 | 334. | -3.3 | 6.46 | 47.8 | 35.7 |
| Circular Structure in Lava in Southwestern Elysium Planitia : ESP_049011_1815 ESP_050145_1815 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.458 | 146. | 2.83 | 26.32 | 40.0 | 29.7 |
| Steep-Front Deposit on Crater Floor in Northern Arabia Terra: ESP_049293_2140 ESP_049359_2140 (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 | 33.61 | 3.59 | -1.5 | -17.5 | 60.0 | 59.9 |
| Concentric Craters : ESP_049154_2185 ESP_049642_2185 (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 | 38.17 | 197. | -4.9 | -20.3 | 65.7 | 59.8 |
| Rifts and Pitted Cones in Utopia Planitia : ESP_049039_2110 ESP_057782_2110 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.70 | 97.8 | 1.95 | 11.30 | 60.7 | 61.2 |
| Polar Pits: Are They Active?: PSP_009834_2645 PSP_009873_2645 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.55 | 134. | -14. | -0.41 | 64.3 | 63.9 |
| Obstacles and Wakes in Lava: ESP_048745_2095 ESP_049378_2095 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.11 | 204. | 7.61 | -7.57 | 62.5 | 55.5 |
| Better Preserved on Mars than on Earth: ESP_014096_1975 ESP_020043_1975 (Interval in Earth days: 464) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.12 | 73.0 | 1.87 | 13.55 | 48.6 | 54.0 |
| Monitoring Temporal Changes in Danielson Crater: ESP_048621_1885 ESP_048476_1885 (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 | 8.265 | 352. | 5.74 | -4.42 | 48.6 | 50.6 |
| Layers and Spider Terrain : ESP_048726_1020 ESP_048990_1020 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -77.9 | 23.5 | 6.68 | -14.2 | 57.4 | 60.1 |
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