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.
| Polar Crater with Summer Ice and Central Uplift: ESP_018479_2460 ESP_019323_2460 (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 | 65.47 | 283. | 3.50 | -8.43 | 51.3 | 61.4 |
| Seasonal Monitoring of Sublimation in Gypsum Source Region: ESP_018335_2600 ESP_018309_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 | 79.97 | 240. | 8.59 | -8.95 | 57.8 | 58.7 |
| Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater: ESP_018268_2335 ESP_033854_2335 (Interval in Earth days: 1215) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.34 | 289. | -4.9 | 20.21 | 46.1 | 47.4 |
| Layered Terrain in Aeolis Planum: ESP_018181_1730 ESP_018893_1730 (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 | -6.83 | 152. | -5.0 | 11.41 | 58.6 | 56.8 |
| Relatively Young Crater Ejecta and Apron in Deuteronilus Mensae: ESP_018423_2230 ESP_019056_2230 (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 | 42.74 | 18.1 | 3.74 | -12.5 | 44.0 | 50.4 |
| North Polar Residual Cap: ESP_018289_2655 ESP_018593_2655 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.19 | 34.7 | 5.01 | -9.35 | 61.3 | 63.9 |
| Lava Channel and Cataract in South-Central Elysium Planitia: ESP_018339_1820 ESP_018194_1820 (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 | 2.117 | 157. | -0.8 | -16.4 | 53.3 | 54.4 |
| Dark Outcrop: ESP_018292_1780 ESP_019492_1780 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.92 | 0.09 | 11.0 | -12.0 | 54.7 | 55.9 |
| 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 |
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