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.
| Gully Monitoring and Topography: ESP_069895_2350 ESP_070528_2350 (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 | 54.55 | 305. | 5.90 | -17.6 | 49.5 | 49.6 |
| Pitted Material and Mounds in Chryse Planitia: ESP_069723_2215 ESP_070013_2215 (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 | 40.95 | 326. | -8.8 | 3.579 | 49.2 | 47.2 |
| Layering in Western Arabia Terra: ESP_069933_1900 ESP_070856_1900 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.694 | 355. | 4.27 | -17.8 | 53.3 | 55.2 |
| Hills in Phlegra Montes: ESP_069729_2190 ESP_089007_2190 (Interval in Earth days: 1502) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.59 | 162. | -5.9 | 8.183 | 48.8 | 45.0 |
| Mounds in Western Oxia Colles: ESP_069802_2005 ESP_069657_2005 (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 | 20.16 | 330. | 8.76 | -7.69 | 49.3 | 50.3 |
| Scalloped Depressions in Utopia Planitia: ESP_069692_2290 ESP_069982_2290 (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 | 48.45 | 90.9 | -4.2 | 10.12 | 49.7 | 47.4 |
| Hill Southeast of Jezero Crater: ESP_069719_1985 ESP_070365_1985 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.19 | 78.2 | -3.7 | 7.67 | 50.8 | 50.0 |
| Exposed Cliff of Stratified Deposits in Melas Chasma: ESP_069751_1670 ESP_070041_1670 (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 | -12.8 | 287. | 0.04 | 17.69 | 64.1 | 64.2 |
| Possible Geological Contact Between Two Units: ESP_069685_1735 ESP_069342_1735 (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 | -6.56 | 289. | -3.1 | 7.599 | 60.5 | 56.3 |
| Possible Angular Unconformity in Zephyria Planum Stratigraphy: ESP_069835_1775 ESP_069413_1775 (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 | -2.28 | 152. | 8.88 | -6.79 | 58.1 | 56.1 |
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