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.
| North Polar Erg Changes: ESP_028055_2605 ESP_028029_2605 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.17 | 191. | 16.3 | -0.45 | 66.3 | 66.9 |
| Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor: ESP_027969_1635 ESP_028325_1635 (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 | -16.2 | 54.6 | -23. | -4.61 | 62.8 | 60.0 |
| Recent Crater on Northern Plains: ESP_027986_2390 ESP_033933_2390 (Interval in Earth days: 463) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 58.50 | 297. | 3.48 | -14.9 | 54.8 | 52.3 |
| North Polar Gypsum Dunes: ESP_027820_2610 ESP_027912_2610 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.93 | 138. | -6.3 | 7.587 | 65.1 | 65.4 |
| Extensive Outcrops of Rhythmic Stratigraphy in Arabia Terra: ESP_027918_1905 ESP_027984_1905 (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 | 10.30 | 1.23 | 3.76 | -15.5 | 49.8 | 51.5 |
| Sinuous Ridge on Crater Wall in Aeolis Region: ESP_027807_1765 ESP_035112_1765 (Interval in Earth days: 569) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.70 | 153. | -4.5 | 12.46 | 55.5 | 54.4 |
| Landforms in Simud Valles in CTX G16_024570_1921_XN_12N038W: ESP_027814_1940 ESP_028592_1940 (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 | 14.01 | 321. | -16. | 6.131 | 50.1 | 52.1 |
| Possible Future Landing Site in Cerberus Palus: ESP_028005_1870 ESP_034532_1870 (Interval in Earth days: 509) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.749 | 146. | 5.47 | 26.39 | 50.8 | 44.3 |
| High-Latitude Exposure of North Polar Layered Deposits: ESP_028001_2680 ESP_019286_2680 (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 | 87.93 | 205. | -13. | -22.6 | 72.3 | 74.2 |
| Flow Boundary in Elysium Planitia: ESP_028149_2085 ESP_028215_2085 (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 | 28.29 | 172. | 4.18 | -12.8 | 49.0 | 51.1 |
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