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.
Lava Channel on the North Flank of Ascraeus Mons: ESP_018520_1920 ESP_018665_1920 (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 | 11.95 | 254. | -4.6 | 13.12 | 49.3 | 48.3 |
Lobate Flow Front in Kasei Valles: ESP_018730_1905 ESP_019231_1905 (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 | 10.46 | 282. | -7.1 | 12.28 | 50.5 | 50.1 |
Layered Terrain in Aeolis Planum: ESP_018603_1755 ESP_019592_1755 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.68 | 150. | 5.39 | -11.1 | 56.5 | 56.6 |
Milankovic Crater: ESP_018785_2345 ESP_019220_2345 (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 | 54.20 | 212. | 5.45 | 25.97 | 49.2 | 52.3 |
Crater Floor: ESP_018584_1795 ESP_019085_1795 (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 | -0.64 | 309. | -5.9 | 14.73 | 55.2 | 53.4 |
Gullied Wall of Impact Crater: ESP_018571_2440 ESP_018703_2440 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 63.74 | 291. | 7.48 | -10.3 | 50.9 | 53.4 |
Gemina Lingula Scarp with Outcrop of Layered Deposits and Unconformities: ESP_018778_2605 ESP_018897_2605 (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 | 80.23 | 26.7 | 6.03 | -9.11 | 61.6 | 63.8 |
Cangwu Crater: ESP_018572_2220 ESP_019073_2220 (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 | 41.84 | 270. | 3.17 | 16.91 | 44.8 | 47.8 |
Acidalia Mensa: ESP_018517_2250 ESP_018649_2250 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.72 | 331. | 2.20 | -25.0 | 45.0 | 48.5 |
Southern Hemisphere Crater with Possible Phyllosilicates: ESP_018737_1665 ESP_019449_1665 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 93.5 | -2.4 | 11.23 | 61.7 | 58.5 |
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