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.
| Exposure of South Polar Layered Deposits: ESP_032123_0925 ESP_032675_0925 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.6 | 107. | 8.70 | 27.7 | 77.6 | 85.1 |
| South Polar Residual Cap in Late Summer: ESP_032408_0920 ESP_032657_0920 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.9 | 263. | 8.07 | 19.64 | 82.9 | 85.7 |
| Pitted Terrain Associated with Lava Flow: ESP_032395_2070 ESP_032672_2070 (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 | 26.74 | 170. | -0.5 | -26.7 | 46.1 | 45.3 |
| Exposure of South Polar Layered Deposits: ESP_032238_0920 ESP_032476_0920 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.9 | 158. | 27.6 | 21.28 | 77.9 | 82.4 |
| Layered Materials on Northeast Hellas Region Rim: ESP_032425_1525 ESP_032359_1525 (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 | -27.2 | 78.3 | -1.1 | 21.31 | 38.0 | 35.6 |
| Terra Cimmeria Intra-Crater Barchan Dune Changes: ESP_032475_1235 ESP_032607_1235 (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 | -56.0 | 157. | 1.83 | -25.4 | 57.2 | 61.0 |
| Scarp in South Polar Layered Deposits: ESP_032255_0915 ESP_041210_0915 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.2 | 61.8 | 26.8 | 17.1 | 78.6 | 81.8 |
| Crater with Lineae and Gullies: ESP_032197_1415 ESP_032619_1415 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.1 | 184. | 3.43 | -17.2 | 40.5 | 48.0 |
| Possible Exposure of South Polar Layered Deposits: ESP_032268_0910 ESP_032295_0910 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.7 | 90.3 | 23.9 | 20.73 | 79.5 | 80.4 |
| Gullies with Bright Deposits in Dao Vallis: ESP_032385_1455 ESP_024328_1455 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.3 | 92.3 | -10. | 22.94 | 41.8 | 51.1 |
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