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.
| Possible Low-Calcium Pyroxene in Nili Fossae: PSP_008426_2025 PSP_009138_2025 (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 | 22.37 | 74.8 | 8.95 | -17.4 | 42.5 | 46.8 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009243_2675 PSP_009297_2675 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.62 | 13.0 | -5.1 | -13.9 | 62.9 | 63.0 |
| 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 |
| Cerberus Fossae: PSP_008752_1865 PSP_009108_1865 (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 | 6.222 | 174. | 8.31 | -1.93 | 50.1 | 51.9 |
| Layered Deposits in Crater in Arabia Terra: PSP_008520_2085 PSP_009232_2085 (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 | 28.00 | 27.9 | 1.13 | -16.8 | 42.3 | 45.8 |
| Characterize Surface Hazards and Science of Possible MSL Rover Landing Site: PSP_008716_2015 PSP_008782_2015 (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 | 21.01 | 74.5 | 20.1 | -5.18 | 42.9 | 45.2 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009240_2675 PSP_009320_2675 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.36 | 114. | -6.0 | -15.0 | 62.5 | 63.0 |
| Dark Materials on Block in Olympus Mons Aureole: PSP_008935_1975 ESP_016372_1975 (Interval in Earth days: 580) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.33 | 217. | -8.1 | 5.979 | 47.1 | 40.0 |
| Characterize Surface Hazards and Science of MSL Rover Landing Site: PSP_008218_1815 PSP_008719_1815 (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 | 1.522 | 357. | 13.4 | -4.22 | 49.6 | 53.4 |
| Central Peak and Floor of Large Crater West of Schiaparelli Crater: PSP_008613_1760 PSP_008969_1760 (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 | -3.93 | 12.2 | 1.91 | -18.6 | 55.6 | 58.3 |
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