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.
| Ridges in Meridiani Planum: ESP_025386_1800 ESP_025663_1800 (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 | 0.029 | 5.68 | -8.1 | -29.6 | 46.6 | 50.5 |
| Colorful Layers in Nili Fossae: ESP_026992_2025 ESP_027691_2025 (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 | 22.13 | 77.1 | 7.52 | -9.02 | 43.3 | 47.3 |
| Active Sand Abrasion in the Northern Polar Region of Mars: ESP_026839_2550 ESP_027248_2550 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.88 | 279. | 6.39 | -8.32 | 53.3 | 56.2 |
| Layered Material Cut by a Valley Connected to East Jezero Crater: ESP_026359_1990 ESP_028535_1990 (Interval in Earth days: 169) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.68 | 78.5 | 8.83 | -12.7 | 42.7 | 53.3 |
| Intersection of Cerberus Fossae and Broad Channel: ESP_026778_1890 ESP_026422_1890 (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 | 8.767 | 161. | 7.46 | -5.38 | 48.0 | 48.0 |
| Cones at Edge of North Polar Layered Deposits: ESP_026694_2605 ESP_026602_2605 (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 | 80.44 | 268. | 7.91 | -6.06 | 56.4 | 57.1 |
| Possible Future Landing Site in Sabrina Vallis Delta: ESP_026601_1920 ESP_034605_1920 (Interval in Earth days: 623) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.68 | 313. | 3.61 | 21.97 | 46.6 | 43.1 |
| Dunes and North Polar Outlier in MOC Image R03-00181: ESP_026963_2595 ESP_026660_2595 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.21 | 124. | 13.6 | -1.03 | 56.0 | 56.1 |
| Possible Future Landing Site in Mawrth Vallis: ESP_026600_2060 ESP_034736_2060 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.53 | 339. | -0.1 | -23.6 | 42.1 | 43.7 |
| Ridges in Meridiani Planum: ESP_026718_1825 ESP_026362_1825 (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 | 2.679 | -0.4 | 11.8 | -0.58 | 50.8 | 50.7 |
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