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.
| Layers and Dark Dunes: ESP_039581_1520 ESP_049009_1520 (Interval in Earth days: 735) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.7 | 203. | -0.5 | 15.81 | 41.2 | 30.4 |
| Prehnite Deposits in Northwest Hellas Region: ESP_039982_1535 ESP_040272_1535 (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 | -26.2 | 56.3 | -5.4 | 20.34 | 37.3 | 33.2 |
| Exposure of South Polar Layered Deposits: ESP_040177_0935 ESP_040295_0935 (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 | -86.4 | 183. | -0.4 | 10.83 | 67.1 | 67.1 |
| Crater on South Polar Layered Deposits: ESP_040269_0970 ESP_040519_0970 (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 | -82.9 | 176. | -17. | 4.772 | 66.0 | 67.1 |
| Enigmatic Surface Morphology in Northwest Syrtis Major Region: ESP_040008_2035 ESP_040074_2035 (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 | 23.33 | 59.7 | 0.00 | -21.2 | 60.0 | 60.5 |
| Sinuous Ridge in Argyre Region: ESP_039933_1240 ESP_048860_1240 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.8 | 318. | 2.08 | -7.99 | 44.6 | 43.1 |
| South Polar Layered Deposits: ESP_040126_1005 ESP_040073_1005 (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 | -79.5 | 102. | -1.6 | 14.54 | 60.9 | 59.6 |
| Southern Mid-Latitude Crater: ESP_039983_1390 ESP_074837_1390 (Interval in Earth days: 2716) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.4 | 30.1 | 4.78 | -9.11 | 38.1 | 43.1 |
| Candidate Landing Site for 2020 Mission in Oyama Crater: ESP_040090_2035 ESP_049294_2035 (Interval in Earth days: 717) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.32 | 340. | 7.12 | -26.4 | 58.7 | 53.3 |
| Crater on South Polar Layered Deposits: ESP_040294_1005 ESP_040347_1005 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -79.4 | 194. | -1.5 | -17.4 | 62.1 | 63.7 |
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