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.
| North Polar Crater Change Detection: ESP_018471_2645 ESP_018498_2645 (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 | 84.32 | 120. | -0.4 | -16.8 | 62.0 | 63.1 |
| Northern Chryse Region: ESP_018346_2125 ESP_018201_2125 (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 | 32.18 | 322. | -3.5 | -15.8 | 44.0 | 44.6 |
| Well Developed Hollows and Ridges in Nilosyrtis Region Crater: ESP_018144_2185 ESP_018856_2185 (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 | 37.98 | 75.6 | 6.46 | 17.99 | 42.1 | 45.1 |
| Central Structure and Layering of a Large Impact Crater: ESP_018263_2230 ESP_018751_2230 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.58 | 67.3 | -5.3 | -27.4 | 43.9 | 49.1 |
| Cones at Edge of North Polar Layered Deposits: ESP_018295_2580 ESP_026985_2580 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.99 | 263. | -6.6 | -21.3 | 57.3 | 57.6 |
| Distorted Layers in Noctis Labyrinthus Trough: ESP_018190_1720 ESP_018823_1720 (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 | -8.09 | 265. | 6.34 | -16.3 | 58.7 | 59.5 |
| Erosional Surface Features in Arabia Terra: ESP_018488_2120 ESP_019345_2120 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.70 | 46.1 | -5.1 | 17.79 | 44.8 | 48.9 |
| North Polar Residual Cap: ESP_018357_2630 ESP_018305_2630 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.84 | 354. | 4.67 | -19.6 | 60.0 | 61.3 |
| Cones at Edge of North Polar Layered Deposits: ESP_018334_2600 ESP_026641_2600 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.05 | 275. | -5.1 | 10.19 | 58.7 | 56.0 |
| Basal Unit in North Polar Layered Deposits Scarp: ESP_018244_2655 ESP_018403_2655 (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 | 85.33 | 189. | 0.39 | -15.0 | 61.4 | 63.0 |
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