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.
| Flow Front in Amazonis Planitia: PSP_008290_2075 PSP_010281_2075 (Interval in Earth days: 155) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.13 | 188. | 5.71 | -12.2 | 41.5 | 50.9 |
| Unnamed Well-Preserved Crater in Tyrrhena Terra: PSP_008544_1615 PSP_009335_1615 (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 | -18.4 | 98.9 | -6.3 | 11.96 | 65.1 | 66.0 |
| Light-Toned Rock and Scarps in MOC Images R10-03225 and R16-01292: PSP_008877_2165 PSP_009523_2165 (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 | 36.29 | 358. | -8.1 | 13.60 | 43.1 | 43.4 |
| Unnamed Crater North of Hellas Basin: PSP_009244_1575 PSP_009666_1575 (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 | -22.2 | 64.8 | 0.54 | -14.7 | 69.2 | 69.8 |
| Polar Layered Deposits Unconformity: PSP_009219_2650 PSP_009416_2650 (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 | 85.08 | 356. | -8.4 | 6.998 | 60.8 | 60.9 |
| Cones among the Tartarus Montes: PSP_008818_2055 PSP_009029_2055 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.15 | 169. | 6.65 | -10.6 | 43.2 | 45.3 |
| Cratered Cones in Isidis Region: PSP_008887_1985 PSP_009177_1985 (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 | 18.11 | 88.2 | -12. | 9.193 | 47.0 | 46.1 |
| Longitudinally-Aligned Knobs in Athabasca Valles: PSP_008344_1895 PSP_008845_1895 (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 | 9.473 | 156. | 6.05 | -11.6 | 47.0 | 50.3 |
| MSL Candidate Landing Site: PSP_009362_2020 PSP_009507_2020 (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 | 21.69 | 78.8 | -11. | 1.906 | 47.2 | 46.5 |
| Tantalus Fossae: PSP_008959_2400 PSP_008089_2400 (Interval in Earth days: 68) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 59.62 | 271. | 13.5 | 2.058 | 45.5 | 48.0 |
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