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.
| Future Mars Landing Site in Antoniadi Crater: ESP_018105_2045 ESP_018250_2045 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.05 | 63.0 | -0.2 | 13.32 | 44.2 | 43.5 |
| Light-Toned Outcrops in Noctis Region: ESP_017979_1715 ESP_018401_1715 (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 | -8.26 | 267. | -7.1 | -21.7 | 59.6 | 60.6 |
| Repeated Sulfate and Clay Beds in West Gale Crater: ESP_017786_1745 ESP_017931_1745 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.36 | 137. | -13. | 1.249 | 57.9 | 57.2 |
| Valleys and Layering along Melas Region: ESP_018018_1705 ESP_026866_1705 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.55 | 283. | -6.8 | -17.8 | 60.4 | 60.2 |
| Raised Polygonal Ridges and Light-Toned Material in Syrtis Region: ESP_018065_1975 ESP_019133_1975 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.49 | 76.4 | -5.2 | 15.52 | 46.5 | 48.0 |
| Layered Material within Small Crater in Nilosyrtis Mensae: ESP_017907_2125 ESP_053787_2125 (Interval in Earth days: 2796) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.07 | 68.2 | -5.4 | 6.933 | 42.7 | 41.6 |
| Well-Preserved Impact Crater with Ridges: ESP_017975_1705 ESP_025557_1705 (Interval in Earth days: 590) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.51 | 16.4 | 0.77 | 18.29 | 59.9 | 51.6 |
| Shallow Channel Cutting through a Crater in CTX Image: ESP_017740_2230 ESP_024900_2230 (Interval in Earth days: 558) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.79 | 305. | 3.34 | 18.77 | 41.7 | 42.4 |
| Cones at Edge of North Polar Layered Deposits: ESP_017833_2615 ESP_018070_2615 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.25 | 272. | -6.5 | 8.031 | 57.9 | 57.5 |
| Layered Terrain in Aeolis and Zephyria Regions: ESP_017825_1760 ESP_018458_1760 (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 | -3.75 | 149. | 13.9 | -9.22 | 55.2 | 57.1 |
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