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.
| Light-Toned Deposits in Northwest Iani Chaos: ESP_084333_1785 ESP_084768_1785 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.48 | 340. | 3.72 | 19.69 | 41.9 | 36.4 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084338_0965 ESP_084219_0965 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -83.2 | 236. | -5.6 | 8.915 | 65.3 | 63.3 |
| Low Ridge and Topography: ESP_084365_2095 ESP_084576_2095 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.36 | 182. | 4.37 | -10.3 | 61.7 | 59.6 |
| Fresh Impact Crater: ESP_084401_1440 ESP_085324_1440 (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 | -35.7 | 287. | 3.51 | -12.0 | 36.9 | 45.2 |
| Dune Change Detection in Mawrth Vallis: ESP_084201_1980 ESP_084135_1980 (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 | 17.79 | 343. | -5.8 | 20.45 | 55.9 | 55.2 |
| Possible Well-Exposed Overturned Terrain in Crater near Her Desher Vallis: ESP_084321_1550 ESP_084400_1550 (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 | -24.7 | 311. | -7.1 | 25.15 | 36.4 | 33.4 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084263_0975 ESP_084382_0975 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.3 | 114. | 6.76 | -8.57 | 63.1 | 65.3 |
| Fresh Crater with Possible Gullies in Cavi Angusti: ESP_084296_1055 ESP_084810_1055 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.2 | 287. | -5.2 | 9.551 | 58.1 | 63.0 |
| Streamline Feature Surrounding Crater in Ares Vallis: ESP_084162_1985 ESP_084373_1985 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.12 | 327. | -2.4 | -21.9 | 56.4 | 55.0 |
| Crater Walls in Terra Sabaea: ESP_084410_1530 ESP_084990_1530 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.8 | 41.3 | -3.3 | 21.13 | 35.8 | 35.1 |
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