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.
| Layered Deposits in West Candor Chasma: ESP_027288_1750 ESP_027644_1750 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.93 | 282. | -24. | -1.62 | 58.0 | 56.1 |
| Survey Layering and Faulting in Layered Deposits in Melas Chasma: ESP_027367_1690 ESP_027512_1690 (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 | -11.0 | 286. | -16. | 5.998 | 60.8 | 59.1 |
| Crater Exposing Bedrock: ESP_027323_2145 ESP_053788_2145 (Interval in Earth days: 2062) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.07 | 40.8 | -5.2 | 5.106 | 43.9 | 41.7 |
| Bacolor Crater: ESP_027030_2135 ESP_027729_2135 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.04 | 118. | 5.21 | -8.28 | 41.8 | 46.8 |
| Gullies on Central Uplift of Lyot Crater: ESP_027376_2310 ESP_027297_2310 (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 | 50.44 | 29.3 | 10.1 | -13.1 | 45.1 | 46.6 |
| Vents and Flows in Elysium Planitia Flood Lava: ESP_027187_1835 ESP_028308_1835 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.341 | 157. | -1.8 | -13.9 | 51.9 | 53.9 |
| Streamlined Features in Olympica Fossae: ESP_027342_2035 ESP_028463_2035 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.32 | 243. | -7.2 | -16.5 | 45.4 | 53.3 |
| Possible Layered Deposit in Open Basin: ESP_027256_2125 ESP_060183_2125 (Interval in Earth days: 2565) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.25 | 68.8 | 6.35 | -2.95 | 42.6 | 39.2 |
| Gale Crater: ESP_027280_1750 ESP_051253_1750 (Interval in Earth days: 1868) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.73 | 137. | 24.2 | 5.454 | 54.4 | 40.6 |
| Dune Migration: ESP_027343_2610 ESP_027448_2610 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.08 | 199. | -6.8 | 13.48 | 60.5 | 60.2 |
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