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.
Recent Impact Crater Through Medusae Fossae Formation and Flood Lavas: ESP_012234_1820 ESP_012511_1820 (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 | 1.990 | 148. | 22.3 | -6.87 | 55.6 | 56.7 |
Enigmatic Uplift on the Floor of Echus Chasma: ESP_011715_1800 ESP_012203_1800 (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 | -0.05 | 279. | 8.06 | -26.2 | 57.0 | 58.9 |
Iron and Magnesium Phyllosilicates in Terra Sabaea Crater Wall: ESP_012278_1695 ESP_066132_1695 (Interval in Earth days: 4196) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.2 | 31.3 | -3.6 | -22.5 | 54.2 | 48.1 |
Cascading Channel in Noachis Pit Crater in MOC M12-00595: ESP_012411_1320 ESP_014046_1320 (Interval in Earth days: 127) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.5 | 5.30 | -0.5 | 13.90 | 53.5 | 40.9 |
Valley Wall on Tyrrhena Patera: ESP_012539_1580 ESP_085291_1580 (Interval in Earth days: 5669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.8 | 106. | 3.57 | -11.9 | 49.2 | 38.5 |
Large Fan in Porter Crater: ESP_012455_1290 ESP_012745_1290 (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 | -50.8 | 245. | -8.9 | 10.54 | 54.4 | 48.5 |
Contact between Wallrock and Light-Toned Rocks in Ophir Chasma: ESP_011662_1750 ESP_011807_1750 (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 | -4.76 | 287. | 6.98 | 23.57 | 56.8 | 55.2 |
Gully in Crater Wall: ESP_011877_1410 ESP_012510_1410 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.8 | 182. | 3.05 | -13.9 | 59.3 | 51.1 |
Cataracts at the Proximal Ends of Distributaries in Athabasca Valles: ESP_011891_1885 ESP_012313_1885 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.235 | 154. | -7.7 | -19.1 | 60.0 | 60.9 |
Shalbatana Vallis Layering: ESP_011740_1830 ESP_019454_1830 (Interval in Earth days: 601) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.120 | 316. | 8.28 | -8.81 | 57.4 | 54.2 |
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