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.
| Exposed Layers in Olympia Mensae Icy Outliers: ESP_089774_2545 ESP_089787_2545 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.13 | 95.1 | -4.3 | 10.35 | 64.8 | 63.9 |
| Survey of Terrain around Ice-Exposing Crater: ESP_089639_2195 ESP_089507_2195 (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 | 39.10 | 190. | -9.9 | 20.77 | 51.6 | 47.5 |
| Inverted Valley and Rings near Erebus Montes: ESP_089850_2210 ESP_089217_2210 (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 | 40.73 | 187. | 7.54 | 17.77 | 52.6 | 45.6 |
| Iani Chaos: ESP_089660_1780 ESP_089238_1780 (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 | -1.75 | 341. | -6.6 | 6.11 | 57.5 | 56.6 |
| Potential Chloride-Rich Deposit near Mawrth Vallis: ESP_089739_2065 ESP_089884_2065 (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 | 26.05 | 340. | 8.34 | 23.47 | 50.2 | 50.0 |
| 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 |
| 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 |
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