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.
| Glacier-Like Form Terminus into Valley Fill: ESP_085405_2185 ESP_085748_2185 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.97 | 226. | -4.2 | -17.4 | 54.5 | 51.5 |
| Curved Channel near Crater Rim: ESP_085495_2165 ESP_085983_2165 (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 | 35.91 | 289. | -1.3 | -16.0 | 51.8 | 48.1 |
| Ridge-Crater Relationships in Osuga Valles: ESP_085349_1650 ESP_085982_1650 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 321. | -4.2 | 3.855 | 36.6 | 42.7 |
| Triangular Faceted Spurs in East Candor Chasma: ESP_085693_1740 ESP_085838_1740 (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 | -6.03 | 291. | -3.9 | 20.84 | 37.7 | 36.9 |
| Alluvial Fans in Kasei Valles: ESP_085363_2035 ESP_085297_2035 (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 | 23.14 | 294. | 0.51 | 16.99 | 45.1 | 44.7 |
| North Pole Facing Deposit in Crater: ESP_085325_2220 ESP_085813_2220 (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 | 41.70 | 249. | -2.3 | 2.947 | 58.0 | 51.8 |
| Inverted Channel in Noachis Terra: ESP_085571_1600 ESP_085782_1600 (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 | -19.9 | 23.0 | -4.5 | 12.69 | 40.3 | 41.8 |
| Hillslope Shapes on Holden Crater Rim: ESP_085006_1550 ESP_085151_1550 (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 | -24.7 | 325. | 2.17 | 18.92 | 36.0 | 35.9 |
| Streamlined Form and Hill in Marte Vallis: ESP_085156_1980 ESP_085433_1980 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.73 | 185. | 7.29 | -6.33 | 43.5 | 42.2 |
| Raised Glacier-Like Forms in Arabia Terra: ESP_085043_2150 ESP_085109_2150 (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 | 34.67 | 27.6 | 6.88 | -10.0 | 56.2 | 56.3 |
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