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.
| Terrain Southwest of Jovis Tholus: ESP_088411_1960 ESP_088978_1960 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.96 | 239. | 5.80 | -9.01 | 47.5 | 49.9 |
| Structure of Viscous Flow Feature Exposed by Ice Degradation: ESP_088510_2220 ESP_088431_2220 (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 | 41.58 | 51.9 | 11.0 | -13.2 | 42.7 | 44.7 |
| Dunes in Northern Mid-Latitude Crater: ESP_088469_2410 ESP_088548_2410 (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 | 60.69 | 87.7 | 5.29 | 19.86 | 47.3 | 46.3 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088500_2435 ESP_088421_2435 (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 | 62.98 | 320. | 7.80 | -6.45 | 48.1 | 49.1 |
| Alluvial Fans and Terraced Scarps in Kasei Valles: ESP_088541_2025 ESP_088330_2025 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.38 | 291. | -19. | -6.13 | 47.7 | 46.0 |
| Pitted Cones in Aurorae Chaos: ESP_088540_1720 ESP_089107_1720 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.77 | 320. | 3.86 | -8.75 | 60.1 | 60.9 |
| Jezero Crater: ESP_088707_1985 ESP_088773_1985 (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 | 18.47 | 77.5 | 0.57 | -21.6 | 47.7 | 49.7 |
| Stunning Outcrop in Nilosyrtis Mensae: ESP_088681_2160 ESP_088892_2160 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.47 | 65.6 | -5.2 | -14.7 | 44.7 | 46.4 |
| Aeolis Dorsa Inverted Deposits: ESP_088612_1735 ESP_088823_1735 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.35 | 154. | -1.4 | -14.9 | 59.6 | 60.6 |
| Layering in Lucus Planum: ESP_088769_1730 ESP_088980_1730 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.74 | 187. | 5.48 | -6.90 | 59.5 | 60.3 |
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