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.
| Well-Preserved Unnamed Crater North of Valles Marineris: PSP_009288_1685 ESP_062957_1685 (Interval in Earth days: 4182) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.3 | 302. | -6.3 | 7.591 | 62.5 | 59.7 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009240_2675 PSP_009320_2675 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.36 | 114. | -6.0 | -15.0 | 62.5 | 63.0 |
| Eroded Mesa in Western Cydonia Region: PSP_008574_2210 PSP_009497_2210 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.74 | 351. | 4.32 | -13.5 | 41.6 | 45.8 |
| 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 |
| Cerberus Fossae: PSP_008752_1865 PSP_009108_1865 (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 | 6.222 | 174. | 8.31 | -1.93 | 50.1 | 51.9 |
| 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 |
| Anatomy of a Well-Defined Crater Ray Emanating from Gratteri Crater: PSP_008514_1630 ESP_025445_1630 (Interval in Earth days: 1320) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.8 | 197. | -1.3 | -14.6 | 63.5 | 57.2 |
| Stratigraphy in Aureum Chaos: PSP_008443_1760 PSP_008944_1760 (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 | -3.72 | 334. | 9.28 | -8.46 | 54.2 | 57.4 |
| 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 |
| Contact between Differing Mineralogies in West Candor Chasma: PSP_008814_1740 ESP_016317_1740 (Interval in Earth days: 584) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.10 | 283. | -3.0 | -21.3 | 58.0 | 49.5 |
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