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.
| Eroded Layered Deposits on Floor of Large Crater: PSP_008200_1555 ESP_052941_1555 (Interval in Earth days: 3486) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.3 | 132. | 4.01 | 15.14 | 66.2 | 66.6 |
| Very Fresh Small Crater in Arabia Region: PSP_009206_1920 ESP_062941_1915 (Interval in Earth days: 4187) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.71 | 17.8 | 3.16 | -6.38 | 49.2 | 50.5 |
| Hematite in Eos Chasma: PSP_008958_1665 PSP_009380_1665 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 312. | -4.7 | -21.8 | 63.1 | 64.7 |
| Outcrop of Light-Toned Deposit South of Coprates Chasma: PSP_009143_1645 ESP_052737_1645 (Interval in Earth days: 3397) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.1 | 301. | -4.2 | 13.31 | 64.6 | 59.4 |
| Pits along the Claritas Rupes: PSP_008512_1630 PSP_009013_1630 (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 | -16.6 | 251. | 6.29 | -8.58 | 62.9 | 65.6 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009190_2680 PSP_009350_2680 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.89 | 0.19 | -6.5 | -13.7 | 63.4 | 63.4 |
| Unusual Crater on Lobate Deposits North of Hrad Vallis: PSP_008384_2150 ESP_016045_2150 (Interval in Earth days: 597) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.63 | 141. | -6.8 | 9.741 | 42.2 | 41.2 |
| Deposits Layered at Several Scales: PSP_009038_1745 PSP_010027_1745 (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 | -5.54 | 286. | 2.43 | -12.1 | 58.0 | 59.4 |
| Characterize Surface Hazards and Science of Possible MSL Rover Landing Site: PSP_008469_2040 PSP_008825_2040 (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 | 23.95 | 340. | 3.44 | -15.0 | 42.8 | 45.4 |
| Cross-Cutting Fractures in the Utopia Region: PSP_008280_2190 PSP_009005_2190 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.89 | 101. | -7.4 | 7.203 | 42.3 | 42.0 |
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