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.
| Valley Network in THEMIS Image V27422018: ESP_033603_2235 ESP_033682_2235 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.36 | 306. | 2.40 | 26.12 | 45.3 | 42.9 |
| Sinuous Channel in Tharsis Region: ESP_033685_1980 ESP_034041_1980 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.85 | 232. | -8.6 | 3.522 | 39.2 | 39.8 |
| Light-Toned Deposits North of Eberswalde Crater: ESP_033418_1565 ESP_033563_1565 (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 | -23.3 | 326. | -6.7 | 8.036 | 50.7 | 51.9 |
| 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 |
| Dunes in Crater North of Antoniadi Crater: ESP_033454_2065 ESP_033955_2065 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.14 | 57.0 | 1.01 | 22.61 | 39.2 | 37.5 |
| Channels and Central Pit of Terra Cimmeria Crater: ESP_033556_1435 ESP_042299_1435 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.3 | 158. | 21.1 | 1.451 | 59.8 | 60.1 |
| 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 |
| Southern Uzboi Vallis Region: ESP_033484_1480 ESP_033629_1480 (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 | -31.7 | 324. | 10.4 | 23.41 | 56.2 | 57.6 |
| Pit or Crater near Galaxias Chaos: ESP_033332_2155 ESP_042088_2155 (Interval in Earth days: 683) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.10 | 146. | 0.31 | 28.38 | 43.1 | 41.8 |
| Layered Light-Toned Crater-Filling Material in Northwest Hellas Region: ESP_033520_1545 ESP_033454_1545 (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 | -25.2 | 62.0 | -3.2 | 18.61 | 53.2 | 50.8 |
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