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.
| Mojave Crater North Rim : ESP_043598_1880 ESP_044798_1880 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.943 | 327. | 7.51 | 25.77 | 45.2 | 45.3 |
| Cratered Cones within a Flow in Elysium Planitia : ESP_043709_2070 ESP_044408_2070 (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 | 26.67 | 174. | 0 | -19.6 | 40.0 | 42.5 |
| Relation of Flow Inside and Outside of Impact Crater in Tharsis Region : ESP_043588_2015 ESP_044076_2015 (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 | 21.34 | 239. | -5.6 | -27.5 | 41.3 | 44.0 |
| Ophir Chasma : ESP_043560_1755 ESP_042360_1755 (Interval in Earth days: 93) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.62 | 287. | -6.6 | 21.06 | 52.7 | 41.1 |
| Light-Toned Layered Deposits in Valles Marineris : ESP_043731_1655 ESP_043665_1655 (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 | -14.1 | 298. | 7.33 | 27.69 | 58.7 | 57.1 |
| Central Candor Chasma : ESP_043705_1720 ESP_053766_1720 (Interval in Earth days: 783) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.76 | 287. | 4.77 | -7.87 | 54.6 | 57.0 |
| Kasei Valles Lava Flow : ESP_043784_2040 ESP_044760_2040 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.88 | 287. | 7.53 | -25.5 | 40.0 | 44.1 |
| Valley Intersecting Crater in Nepenthes Region : ESP_043685_1895 ESP_044806_1895 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.196 | 112. | -4.0 | -22.1 | 45.7 | 48.5 |
| Smooth and Knobby Terrain in Lyot Crater Ejecta : ESP_043622_2330 ESP_043754_2330 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 52.55 | 27.4 | -8.9 | -29.3 | 43.9 | 45.5 |
| Gullied Crater in Tempe Terra : ESP_043705_2225 ESP_043771_2225 (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 | 41.98 | 282. | -5.5 | -19.7 | 40.5 | 41.7 |
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