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.
| Arsia Mons Reticulate Bedform Change Detection: ESP_025760_1705 ESP_025483_1705 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.50 | 237. | -14. | 10 | 55.4 | 51.5 |
| Well Preserved 7-Kilometer Impact Crater in Utopia Planitia: ESP_025791_1945 ESP_025646_1945 (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 | 14.46 | 104. | 24.6 | 6.969 | 40.6 | 41.4 |
| Flow Draped over Crater Rim Visible in CTX Image : ESP_025563_1975 ESP_025207_1975 (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 | 17.48 | 209. | 15.2 | 2.131 | 39.4 | 38.8 |
| Light-Toned Material along Coprates Chasma Wallrock: ESP_025718_1645 ESP_027696_1645 (Interval in Earth days: 154) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.5 | 303. | -0.2 | 13.09 | 58.0 | 60.8 |
| Pit on Crater Floor with Layered Material: ESP_025767_1515 ESP_034549_1515 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.1 | 47.3 | 2.05 | 20.55 | 67.1 | 66.5 |
| Coimbra Crater Interior Layering: ESP_025571_1840 ESP_060410_1840 (Interval in Earth days: 2714) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.988 | 354. | -7.4 | 8.63 | 46.1 | 40.8 |
| Crater and Fans Embayed by Flow Material in Kasei Valles: ESP_025481_2025 ESP_033340_2025 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.14 | 290. | -14. | -0.15 | 40.8 | 38.4 |
| Channel in Tharsis Region: ESP_025417_1965 ESP_024916_1965 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.19 | 235. | 17.6 | -8.13 | 38.8 | 38.5 |
| Crater Rim: ESP_025631_1825 ESP_035969_1825 (Interval in Earth days: 806) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.346 | 156. | -6.2 | 5.312 | 47.2 | 53.4 |
| Ring-Shaped Feature in Northeastern Acidalia Region: ESP_025663_2280 ESP_026362_2280 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.84 | 355. | 4.36 | -18.8 | 42.2 | 43.4 |
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