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.
| 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 |
| Channel Within Lava Flow Emanating from Aromatum Chaos: ESP_065818_1785 ESP_066227_1785 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.49 | 317. | -2.7 | -25.8 | 53.4 | 51.1 |
| 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 |
| Elongated Collapse Pit in Ceraunius Fossae: ESP_066005_2110 ESP_074143_2110 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.54 | 250. | -3.7 | -15.7 | 71.0 | 72.0 |
| Gully Monitoring and Topography: ESP_065837_1415 ESP_066589_1415 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.0 | 163. | 4.75 | -23.9 | 45.1 | 41.7 |
| USGS Dune Database Entry 2579-573: ESP_065438_1225 ESP_065517_1225 (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 | -57.3 | 257. | -4.7 | 21.47 | 55.7 | 52.7 |
| Avernus Colles: ESP_065520_1785 ESP_074080_1785 (Interval in Earth days: 667) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.43 | 172. | -19. | 8.622 | 56.9 | 55.2 |
| Lava-Filled Crater near Athabasca Valles: ESP_065481_1875 ESP_065969_1875 (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 | 7.224 | 154. | -0.2 | 16.82 | 59.3 | 55.2 |
| Flat Layered Deposits and Candidate Exit Breach in Small Young Crater: ESP_065414_1495 ESP_065480_1495 (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 | -30.3 | 186. | 8.30 | -7.95 | 49.9 | 50.3 |
| Gullies and Arcuate Ridges in Nereidum Montes: ESP_065502_1400 ESP_065436_1400 (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 | -39.5 | 307. | -8.7 | 5.813 | 50.6 | 50.5 |
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