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.
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010153_2675 PSP_010603_2675 (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 | 87.58 | 25.7 | -8.4 | -23.4 | 69.2 | 76.0 |
| Pitted Knob on Ceti Mensa: PSP_010093_1740 PSP_010515_1740 (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 | -5.70 | 284. | -6.5 | -19.4 | 59.0 | 59.7 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010163_2675 PSP_010230_2675 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.26 | 123. | -8.3 | -20.4 | 69.1 | 70.5 |
| Impact Crater on Lava Flow Front in Amazonis Planitia: PSP_010109_1975 ESP_053848_1975 (Interval in Earth days: 3408) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.14 | 204. | -6.4 | 7.576 | 50.7 | 44.4 |
| Possible Carbonates in Nili Fossae: PSP_010074_2020 PSP_010351_2020 (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 | 21.68 | 78.9 | 3.17 | -21.0 | 48.8 | 52.5 |
| Layering Under Crater Ejecta: PSP_009324_1830 ESP_020374_1830 (Interval in Earth days: 861) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.065 | 37.4 | 2.15 | 20 | 53.7 | 53.6 |
| 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 |
| 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 |
| 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 |
| Central Structure of Large Crater in Northern Plains: PSP_009332_2360 ESP_018048_2360 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.61 | 171. | 0 | 16.37 | 46.4 | 44.1 |
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