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.
Coprates Chasma Debris Flow Aprons: PSP_008906_1685 PSP_009763_1685 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.3 | 292. | -6.3 | 18.11 | 61.8 | 60.7 |
Crater with Impressive Wind Streak in Elysium Planitia: PSP_008304_1860 ESP_012919_1860 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.728 | 169. | -2.0 | -11.4 | 49.1 | 55.9 |
Well-Preserved 9-Kilometer Diameter Crater: PSP_008902_1565 PSP_009680_1565 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 43.1 | -5.5 | -19.4 | 69.6 | 70.5 |
Characterize Surface Hazards and Science of Possible MSL Rover Landing Site: PSP_008680_2050 PSP_009260_2050 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.63 | 340. | -11. | 19.88 | 44.5 | 43.4 |
Dune Interaction with Topography in Ganges Chasma: PSP_008536_1725 PSP_009604_1725 (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 | -7.40 | 314. | 8.72 | -5.05 | 56.9 | 60.1 |
Polar Layered Deposits Unconformity: PSP_009203_2625 PSP_009585_2625 (Interval in Earth days: 30) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.34 | 79.7 | -7.1 | 7.321 | 58.9 | 59.8 |
Channels Emanating from Cerberus Fossae: PSP_008660_1945 PSP_009016_1945 (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 | 14.38 | 166. | 4.34 | -12.1 | 46.4 | 48.8 |
Basal Units in North Polar Region: PSP_009134_2645 PSP_009687_2645 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.66 | 157. | -7.5 | 10.32 | 60.3 | 62.1 |
Heimdall Crater West of Phoenix Landing Site: PSP_009079_2485 PSP_009092_2485 (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 | 68.27 | 235. | -1.4 | 17.66 | 50.6 | 49.1 |
Bedrock Exposed in Crater Wall in Acidalia Region: PSP_009036_2250 ESP_062850_2250 (Interval in Earth days: 4193) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.59 | 335. | -3.5 | 15.73 | 43.4 | 45.5 |
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