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.
| Small Shield in Eastern Tharsis Region: ESP_065794_1790 ESP_066757_1790 (Interval in Earth days: 75) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.94 | 252. | 3.39 | -10.0 | 53.4 | 44.7 |
| Recent Crater in Southern Mid-Latitudes: ESP_066067_1350 ESP_066476_1350 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.6 | 8.27 | -1.5 | -22.4 | 44.2 | 43.5 |
| Gullies in Southern Hemisphere Crater: ESP_065915_1410 ESP_066047_1410 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.8 | 195. | -7.9 | -28.7 | 45.3 | 45.6 |
| Ares Vallis: ESP_065791_1920 ESP_066200_1920 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.67 | 333. | -3.6 | -25.0 | 60.4 | 58.6 |
| Gullies Associated with Viscous Debris Apron: ESP_065846_1310 ESP_065978_1310 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.6 | 280. | -0.3 | -20.3 | 47.4 | 47.5 |
| Ridges along Pavonis Mons Caldera Rim: ESP_065992_1810 ESP_073853_1810 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.999 | 248. | 6.46 | 17.64 | 52.4 | 56.1 |
| Drainage Features South of Orson Welles Crater: ESP_066082_1780 ESP_074721_1780 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.05 | 313. | -4.7 | -20.6 | 50.8 | 52.2 |
| Active Gully in Matara Crater: ESP_065789_1300 ESP_065934_1300 (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 | -49.4 | 34.8 | 7.58 | 29.10 | 47.6 | 44.3 |
| Lobate Flows in Phlegra Dorsa: ESP_065810_2130 ESP_075016_2130 (Interval in Earth days: 717) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.59 | 171. | -2.4 | 6.659 | 73.2 | 69.7 |
| Slope Failures in Tempe Terra: ESP_065925_2175 ESP_066057_2175 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.31 | 273. | -9.9 | -28.1 | 76.5 | 77.1 |
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