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.
| Equatorial Layered Deposits and Cyclic Depositional Pattern: ESP_084794_1830 ESP_085216_1830 (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 | 3.083 | 350. | 3.13 | -14.5 | 39.4 | 38.1 |
| Jezero Crater Inlet Valley: ESP_084659_1990 ESP_084949_1990 (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 | 18.65 | 76.0 | -2.9 | 10.01 | 50.4 | 46.1 |
| 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 |
| Gullies: ESP_084122_1355 ESP_084333_1355 (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 | -44.1 | 347. | 1.80 | -16.7 | 40.0 | 41.2 |
| 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 |
| Inverted Fluvial Ridge with Complex Structure: ESP_084266_1830 ESP_084055_1830 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.195 | 9.34 | -0.6 | 25.65 | 45.5 | 46.3 |
| Well-Preserved Impact Crater: ESP_084209_1585 ESP_084644_1585 (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 | -21.0 | 128. | 4.91 | 22.15 | 36.6 | 32.9 |
| 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 |
| 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 |
| 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 |
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