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.
| Inclined Layers on Crater Floor: ESP_033518_1405 ESP_033584_1405 (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 | -39.2 | 117. | 8.25 | -11.1 | 62.1 | 64.2 |
| Enigmatic Channel Carved into the Floor of Mangala Valles: ESP_033686_1635 ESP_033831_1635 (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 | -16.1 | 210. | -23. | -7.27 | 51.4 | 52.2 |
| Light-Toned Layered Deposits Exposed along Ladon Valles Floor: ESP_033642_1585 ESP_033787_1585 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.0 | 330. | -3.9 | 12.32 | 52.4 | 53.4 |
| Monitoring Active Dunes in Arabia Terra: ESP_033456_1830 ESP_033601_1830 (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 | 3.139 | 4.55 | 11.1 | 24.90 | 38.0 | 38.1 |
| Possible Smectite Deposits in Northwest Hellas Region: ESP_033652_1580 ESP_041907_1580 (Interval in Earth days: 643) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.6 | 57.2 | 2.99 | 20.83 | 52.5 | 43.8 |
| 12-Kilometer Diameter Crater with Multiple Pronounced Internal Morphologies: ESP_033317_1945 ESP_033462_1945 (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 | 14.33 | 199. | -1.3 | 12.06 | 37.2 | 36.6 |
| Pit South of Arsia Mons: ESP_033342_1660 ESP_050089_1660 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.8 | 240. | -0.3 | -8.91 | 43.9 | 32.6 |
| Eastern Rim of Well-Preserved Crater on Northern Plains: ESP_033684_2355 ESP_033974_2355 (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 | 55.34 | 253. | -5.1 | 12.28 | 51.7 | 48.1 |
| Colorful Crater Rim in Northeast Hellas Planitia: ESP_033427_1460 ESP_033717_1460 (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 | -33.5 | 81.5 | 3.80 | 28.82 | 56.9 | 59.8 |
| Lava-Embayed Crater in Kasei Valles: ESP_033590_2055 ESP_034078_2055 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.39 | 301. | 26.4 | 0.83 | 36.7 | 39.6 |
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