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.
Head of Lethe Vallis: ESP_086199_1840 ESP_087056_1840 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.785 | 153. | 5.44 | 20.19 | 39.3 | 45.1 |
North-Pole-Facing Deposit in Crater: ESP_086208_2275 ESP_086841_2275 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.24 | 261. | 5.23 | -18.4 | 51.0 | 48.1 |
Mesa Stratigraphy at Terby Crater: ESP_086268_1525 ESP_086835_1525 (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 | -27.1 | 73.7 | 3.54 | -8.39 | 53.5 | 62.3 |
Crater in Cerberus Fossae: ESP_086212_1890 ESP_086858_1890 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.700 | 158. | 4.61 | 25.42 | 38.9 | 41.3 |
Thermophysical Boundary West of Hebrus Valles: ESP_086345_2015 ESP_087123_2015 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.09 | 124. | 5.18 | -9.06 | 39.9 | 43.0 |
Young Impact on Layers in Protonilus Mensae: ESP_086295_2230 ESP_086717_2230 (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 | 42.61 | 46.9 | 5.28 | -12.4 | 47.7 | 46.4 |
Ring-Shaped Mounds in Ceraunius : ESP_086815_2115 ESP_087092_2115 (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 | 31.79 | 249. | 16.7 | -7.37 | 40.6 | 42.5 |
North Pole Facing Deposit in Crater: ESP_086235_2230 ESP_085958_2230 (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 | 42.73 | 248. | -17. | 14.10 | 49.9 | 50.2 |
Margin of Lobate Deposit in Nereidum Montes: ESP_086272_1405 ESP_085903_1405 (Interval in Earth days: 29) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 323. | 23.9 | -13.2 | 60.4 | 56.6 |
Gully and Lobate Glacier Fill of Fresh Looking Crater: ESP_086259_2175 ESP_086826_2175 (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 | 37.33 | 311. | 2.92 | -6.63 | 45.5 | 43.8 |
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