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.
| Layering in Arabia Terra: ESP_067228_1820 ESP_074205_1820 (Interval in Earth days: 544) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.134 | -0.7 | -6.5 | 5.414 | 42.1 | 56.2 |
| Possible Valleys in Small Central Pit Crater: ESP_066992_1875 ESP_067467_1875 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.378 | 317. | 1.60 | -6.73 | 45.8 | 42.9 |
| Flow-Like Feature within Chryse Planitia: ESP_067150_2005 ESP_068034_2005 (Interval in Earth days: 69) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.25 | 324. | 5.99 | 28.83 | 51.4 | 42.8 |
| Circular Features North of Olympus Mons: ESP_067114_2145 ESP_067325_2145 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.23 | 225. | -7.8 | 17.19 | 62.2 | 58.0 |
| Feature on South Polar Layered Deposits: ESP_066960_0920 ESP_067143_0920 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 194. | 11.8 | 22.61 | 71.9 | 73.0 |
| Pasted-on Material on Crater Ejecta: ESP_067006_1855 ESP_057986_1855 (Interval in Earth days: 703) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.595 | 295. | 3.93 | -6.11 | 44.6 | 41.1 |
| Crater near Dao Vallis: ESP_067040_1440 ESP_066209_1440 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.8 | 93.1 | 3.28 | -19.1 | 40.0 | 43.0 |
| Flow Surface with Cones in Tartarus Colles: ESP_067050_2070 ESP_067591_2070 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.78 | 172. | -4.5 | -16.3 | 57.5 | 52.4 |
| Scarp in East Candor Chasma: ESP_067059_1735 ESP_066927_1735 (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 | -6.39 | 291. | -6.2 | 17.46 | 40.1 | 39.1 |
| Sinuous Ridge and Channel Southwest of Capen Crater: ESP_066990_1850 ESP_067333_1850 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.150 | 12.7 | -2.4 | 7.947 | 44.9 | 41.7 |
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