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.
| Look for Change Caused By Mass Wasting Since 2007: PSP_009648_2650 PSP_010097_2650 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.99 | 151. | 2.16 | -12.3 | 62.3 | 67.1 |
| 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 |
| Polar Layered Deposits Unconformity: PSP_010048_2615 PSP_010509_2615 (Interval in Earth days: 36) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.49 | 49.1 | -3.5 | 16.55 | 63.8 | 68.5 |
| Strike Slip Fault in Amazonis Planitia: PSP_009463_2010 PSP_009608_2010 (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 | 20.81 | 200. | -2.4 | 11.28 | 47.0 | 46.3 |
| Distributaries From Athabasca Valles: PSP_009768_1880 PSP_010045_1880 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.721 | 154. | 7.98 | -19.7 | 51.6 | 54.3 |
| Exposure of North Polar Basal Unit: PSP_009945_2645 PSP_010063_2645 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.40 | 343. | -12. | 3.559 | 65.2 | 65.5 |
| Western Rim and Ejecta of Very Young 12-Kilometer Diameter Crater: PSP_009810_2140 PSP_010443_2140 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.45 | 84.2 | 7.72 | -5.93 | 45.6 | 51.8 |
| 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 |
| Pit and Channel on Southwestern Pavonis Mons: PSP_009923_1785 PSP_010213_1785 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.67 | 246. | -21. | 14.06 | 58.1 | 55.7 |
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