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.
| Layered Rocks of Ophir Mensa: ESP_036861_1755 ESP_035516_1755 (Interval in Earth days: 105) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.29 | 286. | -3.4 | -15.2 | 57.3 | 57.8 |
| Northwest Tempe Terra: ESP_036992_2195 ESP_041911_2195 (Interval in Earth days: 384) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.07 | 302. | 6.83 | -6.19 | 52.1 | 48.0 |
| Branching Ridges in Western Arabia Terra: ESP_036832_1895 ESP_036898_1895 (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 | 9.143 | 354. | 17.4 | -6.34 | 51.1 | 53.3 |
| North Polar Basal Unit Exposure: ESP_036862_2645 ESP_072362_2645 (Interval in Earth days: 2766) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.31 | 222. | 0 | 14.33 | 69.8 | 72.7 |
| Crater in Arabia Terra: ESP_037095_2140 ESP_089039_2140 (Interval in Earth days: 4048) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.67 | 11.4 | 6.37 | -5.15 | 52.5 | 46.4 |
| Candidate Future Landing Site: ESP_036925_1985 ESP_037558_1985 (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 | 18.20 | 335. | 0.92 | -14.2 | 51.2 | 57.2 |
| Landforms in Nili Fossae: ESP_036974_2005 ESP_037686_2005 (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 | 20.03 | 78.5 | -11. | 13.84 | 52.3 | 56.1 |
| Well-Preserved Impact Crater: ESP_037144_1925 ESP_055460_1925 (Interval in Earth days: 1427) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.35 | 116. | 5.19 | 20.19 | 52.8 | 51.6 |
| Lower Reaches of Shalbatana Vallis: ESP_036952_1895 ESP_042873_1895 (Interval in Earth days: 462) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.379 | 320. | -6.4 | 8.213 | 53.4 | 41.0 |
| Exposure of North Polar Layered Deposits: ESP_037198_2675 ESP_037197_2675 (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 | 87.39 | 28.1 | -8.0 | -1.68 | 77.3 | 77.5 |
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