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.
| 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 |
| Concentric Ridges Near Alcoves Northwest of Oudemans Crater: PSP_008986_1715 PSP_009408_1715 (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 | -8.27 | 266. | 8.18 | -9.64 | 59.2 | 60.9 |
| Chain of Mounds in the Tharsis Region: PSP_008262_1855 ESP_042652_1855 (Interval in Earth days: 2679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.645 | 237. | -7.4 | -23.4 | 49.3 | 43.3 |
| 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 |
| Terraces in Reull Vallis Walls: PSP_008570_1410 PSP_010139_1410 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.4 | 111. | -3.2 | 10.19 | 79.2 | 76.7 |
| Arcadia Planitia Domes: PSP_008554_2170 PSP_008765_2170 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.67 | 177. | 4.87 | -13.3 | 41.4 | 43.3 |
| Mounds on Lineated Valley Fill: PSP_008308_2160 PSP_008888_2160 (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 | 35.70 | 57.0 | -6.7 | 3.944 | 42.1 | 42.1 |
| Terra Cimmeria: PSP_008780_1735 ESP_044502_1735 (Interval in Earth days: 2784) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.43 | 131. | 2.74 | -11.1 | 57.7 | 56.2 |
| 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 |
| 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 |
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