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.
| Phlegra Montes: ESP_075346_2165 ESP_093055_2165 (Interval in Earth days: 1380) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.21 | 162. | 7.16 | -14.4 | 69.2 | 69.2 |
| Scarp Monitoring: ESP_075270_1190 ESP_075613_1190 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -60.7 | 92.0 | -2.1 | -18.0 | 48.1 | 50.6 |
| Light-Toned Deposits in Iani Chaos: ESP_075366_1795 ESP_075999_1795 (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 | -0.28 | 341. | -1.3 | -14.2 | 44.5 | 39.1 |
| Canyon Floor in East Coprates Chasma: ESP_075407_1650 ESP_075473_1650 (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 | -15.0 | 304. | -4.1 | -21.8 | 38.2 | 39.0 |
| Mounds and Pit on Thick Carbon Dioxide Ice: ESP_075399_0920 ESP_074989_0920 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.1 | 219. | 15.6 | 25.47 | 66.9 | 64.0 |
| Layers at Edge of Pedestal Crater in Tikhonravov Crater: ESP_075364_1940 ESP_076353_1940 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.64 | 35.2 | -7.3 | 2.427 | 53.3 | 41.6 |
| Distal Ramparts of Fresh Impact Crater: ESP_075440_2035 ESP_083840_2035 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.43 | 118. | 4.11 | 17.21 | 58.5 | 62.6 |
| Fractured Rises in Iani Chaos: ESP_075445_1770 ESP_076434_1770 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.79 | 346. | -5.3 | 6.497 | 42.5 | 35.2 |
| Volcanic Flow near Tempe Terra: ESP_075487_2110 ESP_084177_2110 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.56 | 275. | -5.0 | 7.021 | 63.8 | 64.8 |
| Channel and Crater North of Huygens Crater: ESP_075416_1745 ESP_075772_1745 (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 | -5.39 | 57.5 | 0.14 | 18.63 | 41.3 | 36.4 |
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