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.
| Sinuous Channel and Trough in Tharsis Region : ESP_058660_2030 ESP_058370_2030 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.92 | 248. | 11.4 | -7.29 | 43.6 | 48.3 |
| Inverted Carbon Dioxide Topography : ESP_058528_0955 ESP_058488_0955 (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 | -84.1 | 297. | -7.9 | 6.803 | 74.4 | 72.7 |
| Collapse Terrain near Head of Ravi Vallis : ESP_058539_1785 ESP_059040_1785 (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 | -1.48 | 316. | 3.28 | 17.05 | 31.8 | 30.1 |
| South Polar Layered Deposits : ESP_057906_0925 ESP_057891_0925 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.5 | 54.9 | 2.46 | 13.98 | 69.5 | 67.4 |
| Crater Partially Buried by Ejecta from Yuty Crater: ESP_058143_2020 ESP_058855_2020 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.98 | 325. | 7.78 | -1.45 | 49.8 | 41.6 |
| High-Latitude Exposure of South Polar Layered Deposits : ESP_057902_0875 ESP_057888_0875 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.3 | 204. | 8.96 | 1.928 | 70.7 | 70.1 |
| Eastern Portion of Well-Exposed 6-Kilometer Crater in Ladon Valles : ESP_058209_1620 ESP_057998_1620 (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 | -17.6 | 328. | 7.97 | 22.18 | 29.4 | 29.1 |
| East Rim of Well-Preserved Impact Crater : ESP_058124_2005 ESP_067210_2005 (Interval in Earth days: 708) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.21 | 126. | -7.3 | 14.69 | 49.5 | 50.1 |
| Floor of East Candor Chasma : ESP_057973_1735 ESP_057907_1735 (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 | -6.47 | 291. | -8.4 | 5.757 | 35.0 | 34.7 |
| Possible Exposure of South Polar Layered Deposits : ESP_058087_0915 ESP_057640_0915 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.5 | 106. | 23.2 | 16.57 | 69.9 | 66.6 |
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