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.
| Potential Phyllosilicates in Acidalia Region: PSP_009182_2215 PSP_009472_2215 (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 | 41.28 | 309. | -4.4 | 16.00 | 43.6 | 43.0 |
| Exposure of Polar Layered Deposits Not Well Observed by Previous Missions: PSP_009039_2680 PSP_009133_2680 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.00 | 169. | -8.0 | -15.3 | 63.1 | 63.0 |
| Impact Crater Amid the Deuteronilus Mensae: PSP_009021_2245 PSP_009654_2245 (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 | 44.21 | 23.3 | 8.73 | -7.10 | 42.2 | 46.4 |
| Landslides in Ganges Chasma: PSP_009037_1715 PSP_009538_1715 (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 | -8.54 | 315. | -14. | 7.943 | 60.9 | 59.8 |
| Zunil Crater Ray Formed within a Dusty Region: PSP_008225_1830 ESP_018510_1830 (Interval in Earth days: 801) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.916 | 167. | -2.7 | 16.38 | 50.1 | 51.7 |
| Layered Deposits in Crater in Arabia Terra: PSP_008520_2085 PSP_009232_2085 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.00 | 27.9 | 1.13 | -16.8 | 42.3 | 45.8 |
| Merging Lobate Debris Aprons of Deuteronilus Mensae: PSP_008744_2240 PSP_009535_2240 (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 | 43.76 | 29.3 | -6.2 | 15.83 | 43.0 | 43.5 |
| Stratigraphy Exposed in Crater Wall: PSP_009048_1965 PSP_010037_1965 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.47 | 11.6 | -4.7 | -17.5 | 47.5 | 51.5 |
| Central Peak of Bonestell Crater: PSP_008733_2225 ESP_018372_2225 (Interval in Earth days: 752) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.96 | 329. | -2.7 | 11.77 | 42.5 | 43.0 |
| Unnamed Faded Rayed Crater in Elysium Planitia: PSP_009123_2040 ESP_016560_2040 (Interval in Earth days: 579) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.94 | 122. | 3.65 | 21.08 | 44.6 | 38.5 |
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