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.
| Contact between Medusae Fossae Formation and Apollinaris Mons Flank: ESP_065942_1725 ESP_066008_1725 (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 | -7.30 | 173. | 8.42 | -5.76 | 48.9 | 49.3 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_065936_1985 ESP_066147_1985 (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 | 18.19 | 335. | -5.2 | 14.27 | 63.5 | 60.7 |
| Mesa in Low Northern Latitudes: ESP_066046_1900 ESP_073973_1900 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.890 | 213. | 2.52 | -8.89 | 57.1 | 61.0 |
| Layering in Crater: ESP_065840_1220 ESP_065972_1220 (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 | -57.4 | 84.6 | 7.60 | -9.28 | 49.8 | 49.7 |
| Outflow Channel from Morella Crater: ESP_065792_1700 ESP_057880_1700 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.85 | 309. | -13. | 5.997 | 51.0 | 33.6 |
| Hydrated Sulfate-Rich Terrain in Aram Chaos: ESP_066081_1830 ESP_092930_1830 (Interval in Earth days: 2092) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.992 | 339. | -0.1 | -20.4 | 53.1 | 48.0 |
| 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 |
| Gullies Monitoring near Ogygis Undae: ESP_066083_1295 ESP_066571_1295 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -50.2 | 292. | 3.28 | 17.14 | 45.3 | 42.7 |
| Ridge in Eastern Candor Chasma: ESP_065819_1735 ESP_065885_1735 (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 | -6.66 | 291. | -3.2 | -17.7 | 51.2 | 51.6 |
| Patchy Outcrop of Light-Toned Materials: ESP_066023_1480 ESP_074952_1480 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.6 | 127. | -3.7 | 8.269 | 43.4 | 39.7 |
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