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.
| Slope Streaks Beginning at Stratigraphic Layers: PSP_007473_1850 PSP_008264_1850 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.996 | 181. | -5.4 | 5.46 | 43.6 | 48.7 |
| Streamlined Form North of Mangala Valles: PSP_007683_1805 PSP_009542_1805 (Interval in Earth days: 145) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.500 | 207. | -3.0 | -16.3 | 47.1 | 56.6 |
| Possible Chloride Salt Deposit: PSP_007058_1745 ESP_016354_1745 (Interval in Earth days: 724) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.62 | 353. | 4.05 | -22.5 | 42.7 | 49.8 |
| Circular Feature with Layers of Repeated Thickness and Expression: PSP_007427_1820 PSP_007862_1820 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.331 | 357. | -0.1 | 20.72 | 44.2 | 46.5 |
| Western Elysium Planitia Boundary: PSP_008015_1840 PSP_009940_1840 (Interval in Earth days: 150) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.067 | 141. | -0.4 | -16.9 | 47.9 | 55.3 |
| Thermally-Distinct Ridges Seen in THEMIS Images I09390002 and V24116005: PSP_007838_1555 PSP_008840_1555 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.0 | 297. | 3.49 | -19.3 | 62.6 | 70.9 |
| Interaction between Unnamed Crater Ejecta and Pre-Exsisting Terrain: PSP_007681_2000 PSP_008406_2000 (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 | 19.66 | 259. | -6.6 | 23.65 | 41.5 | 41.9 |
| Gullies Possibly Produced by Snow or Ice Melting: PSP_007270_2240 PSP_010487_2240 (Interval in Earth days: 251) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.42 | 319. | -2.8 | 11.76 | 45.5 | 52.4 |
| Central Peak and South Rim of Large Fresh Crater in Isidis Basin: PSP_007107_1900 PSP_009823_1900 (Interval in Earth days: 211) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.02 | 94.3 | 0.07 | -12.8 | 39.2 | 52.4 |
| Recent Crater: PSP_007750_1900 ESP_051001_1895 (Interval in Earth days: 3370) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.637 | 176. | 5.67 | -4.50 | 43.3 | 35.5 |
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