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.
| Candidate Mud Volcanoes Targeted by Zhurong Rover: ESP_076891_2050 ESP_077023_2050 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.74 | 109. | 5.44 | -19.3 | 43.1 | 44.2 |
| Layered Sediments in Southern Arabia Terra: ESP_076750_1835 ESP_076407_1835 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.588 | 1.33 | -2.5 | 17.65 | 37.2 | 35.9 |
| Plateau adjacent to Subsiding Terrain: ESP_076976_1775 ESP_078031_1775 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.32 | 313. | 4.72 | 24.37 | 37.5 | 46.2 |
| Interaction Between Cone and Ejecta : ESP_076922_2250 ESP_077832_2250 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.42 | 341. | -3.8 | 8.962 | 55.0 | 46.2 |
| Floor-Fractured Crater in Elysium Planitia: ESP_076810_1895 ESP_075966_1895 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.398 | 160. | 22.6 | -5.00 | 36.2 | 43.3 |
| Ridges near Vernal Crater: ESP_076737_1835 ESP_076948_1835 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.400 | 355. | 6.13 | 23.18 | 36.4 | 35.6 |
| Smooth Region in Phlegra Montes: ESP_076889_2170 ESP_076691_2170 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.79 | 163. | -4.0 | 27.78 | 50.4 | 50.5 |
| Mounds in Oxia Colles: ESP_076751_2015 ESP_076197_2015 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.10 | 332. | -4.7 | 8.674 | 43.0 | 47.1 |
| Valley South of Ares Vallis: ESP_076896_1890 ESP_076962_1890 (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 | 9.103 | 335. | 8.83 | -5.66 | 37.4 | 38.6 |
| Crater Cross-Section of Pitted Materials with Mafic Spectral Signature: ESP_076703_1405 ESP_076848_1405 (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 | -39.4 | 209. | -1.3 | 24.42 | 49.7 | 50.5 |
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