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.
| Mamers Valles: PSP_009773_2165 ESP_053789_2165 (Interval in Earth days: 3429) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.13 | 14.3 | 5.21 | -4.42 | 45.5 | 42.7 |
| Fresh Santa Fe Crater in Chryse Planitia: PSP_009749_1995 PSP_010382_1995 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.36 | 312. | 3.75 | -11.7 | 47.9 | 52.2 |
| Well-Preserved Crater on a Steep Slope in Tyrrhena Terra: PSP_009824_1610 PSP_010246_1610 (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 | -18.5 | 69.0 | 6.12 | -5.57 | 65.8 | 65.3 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010080_2680 PSP_010856_2720 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.79 | 209. | -8.2 | -6.88 | 68.7 | 80.5 |
| Rayed Thila Crater in Elysium Planitia: PSP_009346_1985 PSP_009491_1985 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.08 | 155. | -5.4 | 8.677 | 47.7 | 47.0 |
| Sapping Features East of Tooting Crater: PSP_010333_2025 PSP_010689_2025 (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 | 22.14 | 208. | -3.9 | 0.754 | 50.8 | 53.1 |
| Central Pit of Large But Well-Preserved Crater: PSP_009585_1660 PSP_010429_1660 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 113. | 5.01 | -19.0 | 63.2 | 63.2 |
| Small Crater on the North Polar Deposits: PSP_009773_2675 PSP_010500_2675 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.25 | 297. | 0.08 | -14.1 | 65.4 | 73.7 |
| Southern Highlands High Thermal Inertia and Spectrally Distinct Materials: PSP_010326_1560 PSP_010471_1560 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.7 | 44.9 | 4.00 | 18.94 | 67.2 | 65.4 |
| Phyllosilicates in Acidalia Region: PSP_009538_2220 PSP_010039_2220 (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 | 41.78 | 309. | 0.48 | 17.37 | 44.8 | 46.8 |
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