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.
| Alluvial Fans in Kasei Valles: ESP_077966_1980 ESP_078032_1980 (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 | 17.91 | 285. | 25.5 | 3.616 | 39.6 | 41.9 |
| Streamlined Mound in Marte Vallis: ESP_077983_1945 ESP_080172_1945 (Interval in Earth days: 171) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.10 | 183. | 4.13 | -10.2 | 42.1 | 51.9 |
| Sulfate-Rich Terrain in Aureum Chaos: ESP_078004_1760 ESP_085586_1760 (Interval in Earth days: 591) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.97 | 332. | 4.77 | -17.2 | 48.3 | 37.9 |
| Light-Toned Deposits in Iani Chaos: ESP_077885_1775 ESP_088671_1775 (Interval in Earth days: 840) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.61 | 342. | 0.44 | 12.21 | 46.7 | 56.6 |
| Ascraeus Mons Southern Caldera Wall: ESP_078165_1910 ESP_078455_1910 (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 | 10.88 | 255. | -2.7 | 22.24 | 44.5 | 44.5 |
| Crater with Gullies: ESP_078122_1470 ESP_086851_1470 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.6 | 355. | -3.6 | 17.84 | 67.4 | 64.6 |
| Traverse Ramp in East Coprates Chasma: ESP_077926_1640 ESP_078361_1640 (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 | -15.6 | 306. | -27. | 4.196 | 55.8 | 58.5 |
| Exposed Stratigraphy in Peraea Cavus Southern Wall: ESP_077960_1500 ESP_078171_1500 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.7 | 95.5 | 24.1 | 12.30 | 61.6 | 65.1 |
| Ascraeus Mons Northeastern Caldera Wall: ESP_077954_1915 ESP_077453_1915 (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 | 11.36 | 256. | 4.63 | -9.42 | 42.5 | 40.6 |
| Well-Preserved 6-Kilometer Impact Crater South of Eos Chasma: ESP_078163_1610 ESP_081420_1610 (Interval in Earth days: 254) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.6 | 313. | 2.38 | 26.26 | 58.3 | 61.3 |
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