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.
| Double Crater: ESP_089603_2125 ESP_089880_2125 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.26 | 93.1 | -1.8 | -20.5 | 49.9 | 54.1 |
| Dune Interaction with Residual Polar Ice: ESP_089800_2600 ESP_089826_2600 (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 | 79.64 | 98.5 | -0.5 | 16.96 | 67.8 | 67.0 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_089726_1975 ESP_089225_1975 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.14 | 336. | 11.0 | -14.0 | 50.8 | 50.8 |
| Kasei Valles Alluvial Fan and Distributary Channels: ESP_089899_2035 ESP_089622_2035 (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 | 23.09 | 293. | -4.0 | 17.28 | 52.5 | 48.8 |
| Potential Rotorcraft Landing Site Characterization: ESP_089771_2185 ESP_089837_2185 (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 | 38.22 | 186. | -8.1 | -22.4 | 52.6 | 54.7 |
| Glacier Layering Revealed by Impact Crater on Viscous Flow Features Surface: ESP_089764_2200 ESP_089487_2200 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.61 | 17.6 | -8.7 | 10.06 | 52.8 | 48.4 |
| Kasei Valles Alluvial Fans and Flood Terrace: ESP_089820_2025 ESP_089675_2025 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.03 | 290. | -0.2 | -16.9 | 51.7 | 52.1 |
| Features around Crater in Terra Sabaea: ESP_089842_2165 ESP_089565_2165 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.09 | 50.5 | -24. | -6.66 | 54.5 | 50.2 |
| Closed Fretted Terrain Valley: ESP_089724_2185 ESP_089790_2185 (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 | 38.34 | 28.0 | 6.60 | -9.01 | 50.9 | 52.9 |
| Avalanche Scarp: ESP_089821_2640 ESP_089848_2640 (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 | 83.78 | 237. | -3.9 | -21.3 | 70.6 | 72.2 |
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