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.
| Mid-Latitude Crater with Steep Slopes: ESP_063846_2205 ESP_070033_2205 (Interval in Earth days: 482) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.01 | 140. | 23.6 | 3.324 | 56.0 | 47.1 |
| Candidate Landing Site in 2020 and Sample Return Missions at Jezero Crater: ESP_063809_1985 ESP_064231_1985 (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 | 18.10 | 77.1 | -0.6 | -16.2 | 54.3 | 59.4 |
| Northern Continuous Ejecta Boundary of Noord Crater in Noachis Terra: ESP_063997_1610 ESP_064063_1610 (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 | -18.9 | 348. | 2.28 | -20.1 | 60.7 | 62.1 |
| Light-Toned Layered Deposits: ESP_064026_1740 ESP_064171_1740 (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 | -6.01 | 275. | -0.6 | 15.26 | 57.5 | 56.3 |
| Crater in Arabia Terra: ESP_063851_2240 ESP_063429_2240 (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 | 43.63 | 7.62 | -7.0 | 7.59 | 59.9 | 52.6 |
| North Polar Residual Ice and Defrosting Dunes: ESP_063899_2615 ESP_063873_2615 (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 | 81.63 | 110. | 8.93 | -5.93 | 77.0 | 77.4 |
| Jezero Crater: ESP_064165_1985 ESP_072422_1985 (Interval in Earth days: 643) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.87 | 77.3 | 0.68 | -25.2 | 57.5 | 55.9 |
| Transect along Baetis Chasma: ESP_064078_1755 ESP_064223_1755 (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 | -4.29 | 295. | 6.84 | 21.86 | 56.6 | 55.5 |
| Blocky Terrain in Acidalia Planitia: ESP_064011_2250 ESP_064090_2250 (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 | 44.48 | 319. | -6.3 | 18.08 | 62.6 | 61.8 |
| Candidate Landing Site in 2020 Mission at Jezero Crater: ESP_064020_1980 ESP_063954_1980 (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 | 18.03 | 76.9 | -7.6 | 14.15 | 56.7 | 54.3 |
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