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.
| Layered Flow Ejecta in Terra Cimmeria: ESP_018379_1695 ESP_018880_1695 (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 | -10.4 | 146. | 6.62 | 27.95 | 60.0 | 57.5 |
| Cracks and Fans on Dunes: ESP_018404_2610 ESP_018865_2610 (Interval in Earth days: 36) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.96 | 156. | 6.25 | 24.73 | 59.0 | 62.0 |
| 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 |
| 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 |
| Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae: ESP_018225_2275 ESP_018146_2275 (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 | 47.18 | 22.7 | 5.82 | -17.3 | 43.5 | 45.3 |
| 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 |
| 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 |
| 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 |
| 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 |
| Dissected Crater Central Mound: ESP_018218_1755 ESP_028688_1765 (Interval in Earth days: 815) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.27 | 222. | -8.8 | 10.23 | 57.4 | 54.0 |
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