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.
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084340_0950 ESP_084301_0950 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.8 | 177. | 8.92 | -6.44 | 65.6 | 66.5 |
| North Branch of Kasei Valles East of Labeatis Mensa: ESP_084493_2060 ESP_084058_2060 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.76 | 287. | 8.43 | -6.75 | 57.0 | 63.3 |
| Olivine and Hydrated Mineral-Rich Terrain in Nili Fossae: ESP_084158_2025 ESP_084382_2025 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.23 | 76.9 | -8.9 | 24.45 | 59.7 | 55.0 |
| Light-Toned Deposits in Northwest Iani Chaos: ESP_084333_1785 ESP_084768_1785 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.48 | 340. | 3.72 | 19.69 | 41.9 | 36.4 |
| Potential Fan Deposit in Crater near Mawrth Vallis: ESP_084425_1990 ESP_084491_1990 (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 | 18.82 | 343. | 19.4 | -2.18 | 52.3 | 52.7 |
| Fresh Crater with Possible Gullies in Cavi Angusti: ESP_084296_1055 ESP_084810_1055 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.2 | 287. | -5.2 | 9.551 | 58.1 | 63.0 |
| Intersecting Flow Fronts and Channels: ESP_084101_1845 ESP_084391_1845 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.307 | 194. | 1.77 | 11.16 | 48.0 | 43.8 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084261_0935 ESP_084247_0935 (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 | -86.5 | 200. | 0.09 | 14.22 | 67.1 | 65.7 |
| Light-Toned Deposits in Small Depression in Iani Chaos: ESP_084122_1760 ESP_092073_1760 (Interval in Earth days: 619) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.84 | 342. | 2.11 | -23.7 | 43.3 | 54.1 |
| Inverted Channel in Noachis Terra: ESP_084292_1605 ESP_084503_1605 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.2 | 22.4 | -3.9 | -18.4 | 36.9 | 36.7 |
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