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.
| Big Fresh Crater with a Gullied Central Peak: PSP_007845_2190 PSP_008135_2190 (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 | 38.53 | 99.2 | -5.6 | 5.818 | 42.3 | 41.1 |
| Perplexing Landforms on Hellas Basin Floor: PSP_007135_1400 ESP_016088_1400 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 56.8 | -4.2 | 16.93 | 64.5 | 65.2 |
| Region Showing Differentially-Eroded Distal Fan Deposits: PSP_007688_1575 PSP_008545_1575 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.0 | 72.9 | 6.99 | -15.6 | 59.4 | 68.1 |
| Fresh Double Layer Ejecta Crater in Northern Plains: PSP_007736_2345 PSP_008303_2345 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.37 | 190. | 8.23 | -7.73 | 47.0 | 45.9 |
| Cones Among the Tartarus Montes: PSP_007671_2065 PSP_007882_2065 (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 | 26.03 | 170. | 7.68 | -8.70 | 39.9 | 41.8 |
| Finely-Layered Deposits in Henry Crater: PSP_008072_1905 PSP_009153_1905 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.17 | 24.0 | 0.27 | 15.57 | 45.7 | 48.8 |
| Unusually Large Gullies on Equator-Facing Slope of Crater: PSP_007692_2235 PSP_008694_2235 (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 | 43.35 | 315. | 2.62 | -10.7 | 43.2 | 43.3 |
| Crater with Gullies Seen in MOC Image E14-02164: PSP_007250_1415 ESP_015979_1415 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 155. | 5.87 | -13.0 | 64.8 | 64.5 |
| Unnamed Small Rayed Crater in Hesperia Region: PSP_008135_1520 PSP_008425_1520 (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 | -27.9 | 108. | -4.0 | 6.037 | 68.6 | 70.2 |
| Contact between Two Different Units in Ganges Mensa: PSP_007666_1725 PSP_008022_1725 (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 | -7.65 | 311. | 6.47 | -5.41 | 50.4 | 54.5 |
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