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.
| Large Alluvial Fan in Kasei Valles: ESP_089846_2065 ESP_089991_2065 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.23 | 300. | -2.1 | 14.95 | 51.9 | 51.7 |
| Volcanic Cones in Ceraunius Fossae: ESP_089650_2050 ESP_089927_2050 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.57 | 250. | 6.19 | -14.8 | 49.8 | 53.6 |
| Valley Incision in Crater: ESP_089765_2095 ESP_090253_2095 (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 | 29.13 | 349. | 14.9 | -1.24 | 49.8 | 56.0 |
| Potential Chloride-Rich Deposit near Mawrth Vallis: ESP_089739_2065 ESP_089884_2065 (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 | 26.05 | 340. | 8.34 | 23.47 | 50.2 | 50.0 |
| Survey of Terrain around Ice-Exposing Crater: ESP_089639_2195 ESP_089507_2195 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.10 | 190. | -9.9 | 20.77 | 51.6 | 47.5 |
| Crater in Arabia Terra: ESP_089804_2205 ESP_090160_2205 (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 | 39.96 | 7.23 | -21. | -7.62 | 54.5 | 57.6 |
| Potential Rotorcraft Landing Site Characterization: ESP_089771_2185 ESP_089837_2185 (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 | 38.22 | 186. | -8.1 | -22.4 | 52.6 | 54.7 |
| Fretted Terrain Valley Head in Coloe Fossae: ESP_089723_2160 ESP_090290_2160 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.80 | 56.1 | 2.51 | 18.35 | 50.9 | 56.0 |
| Inverted Valley and Rings near Erebus Montes: ESP_089850_2210 ESP_089217_2210 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.73 | 187. | 7.54 | 17.77 | 52.6 | 45.6 |
| Light-Toned Exposures on Floor of Coprates Chasma: ESP_089780_1645 ESP_090057_1645 (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 | -15.2 | 306. | 6.84 | -14.8 | 62.3 | 62.9 |
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