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.
| Crater in Arabia Terra: ESP_072596_2195 ESP_077238_2195 (Interval in Earth days: 361) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.40 | 1.64 | -2.6 | -24.5 | 58.1 | 50.5 |
| Extra-Crater Sinuous Ridge: ESP_072693_2240 ESP_072772_2240 (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 | 43.67 | 232. | -2.8 | 21.12 | 60.6 | 59.7 |
| Layers in and over Mawrth Vallis: ESP_072689_2015 ESP_072768_2015 (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 | 21.28 | 344. | -4.1 | 27.08 | 56.2 | 54.1 |
| Mounds in Oxia Colles: ESP_072597_2045 ESP_072452_2045 (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 | 24.46 | 336. | -1.7 | -11.3 | 55.4 | 54.9 |
| Small Delta or Fan: ESP_072753_2090 ESP_080362_2090 (Interval in Earth days: 593) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.81 | 36.4 | -3.1 | -16.6 | 57.7 | 49.7 |
| Pitted Cone on Mesa in Isidis Planitia: ESP_072580_1970 ESP_072870_1970 (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 | 16.89 | 81.3 | -1.0 | 21.42 | 54.9 | 55.1 |
| Layered Light-Toned Deposits: ESP_072668_1540 ESP_072958_1540 (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 | -25.7 | 203. | 1.43 | 25.30 | 64.9 | 60.8 |
| Pitted Crater Ejecta: ESP_072417_2350 ESP_072707_2350 (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 | 54.85 | 206. | -5.6 | 6.158 | 60.5 | 64.1 |
| Small Delta or Fan: ESP_072751_1540 ESP_081573_1540 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.6 | 97.5 | 0.94 | 24.57 | 64.3 | 63.2 |
| Deposits in Ganges Chasma: ESP_072664_1715 ESP_072743_1715 (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 | -8.58 | 311. | -6.8 | 28.24 | 59.5 | 56.4 |
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