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.
| Noctis Labyrinthus: ESP_047504_1740 ESP_059016_1740 (Interval in Earth days: 897) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.12 | 254. | 0 | -19.0 | 49.8 | 32.9 |
| Crater in Arabia Terra: ESP_047446_1900 ESP_065393_1900 (Interval in Earth days: 1398) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.647 | 36.3 | 2.18 | -7.22 | 55.0 | 61.2 |
| Central Resen Crater: ESP_047549_1520 ESP_057228_1520 (Interval in Earth days: 754) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.9 | 108. | 1.35 | -27.1 | 47.5 | 39.3 |
| Impact Crater North of Hellas Region: ESP_047590_1520 ESP_048658_1520 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 68.8 | 5.92 | -13.0 | 46.7 | 35.3 |
| Residual South Polar Cap Deposits: ESP_047488_0930 ESP_047503_0930 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.7 | 16.1 | 8.52 | -7.40 | 73.4 | 75.7 |
| Fresh Rayed Crater on Slope into Hadriaca Patera: ESP_047576_1500 ESP_048723_1500 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.4 | 92.3 | -4.4 | 10.48 | 47.8 | 32.9 |
| Potential Dike Associated with Aromatum Chaos: ESP_047449_1785 ESP_048451_1785 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.30 | 316. | -2.1 | 3.725 | 51.5 | 44.7 |
| Terminal Lobes of Landslide or Large Debris Flow in Melas Chasma: ESP_047450_1685 ESP_048953_1685 (Interval in Earth days: 117) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 290. | -2.4 | 15.23 | 49.3 | 33.6 |
| Polygonal Shapes Southwest of Olympus Mons: ESP_047611_1915 ESP_048046_1915 (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 | 11.49 | 211. | 0 | 27.88 | 56.2 | 53.4 |
| Layers in Crater Southwestern Arabia Terra: ESP_047421_1890 ESP_064036_1890 (Interval in Earth days: 1295) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.862 | -0.8 | 0.83 | 18.37 | 54.8 | 54.4 |
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