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.
| Relation of Flow Inside and Outside of Impact Crater in Tharsis Region : ESP_043588_2015 ESP_044076_2015 (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 | 21.34 | 239. | -5.6 | -27.5 | 41.3 | 44.0 |
| Light-Toned Layered Deposits in Valles Marineris : ESP_043731_1655 ESP_043665_1655 (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 | -14.1 | 298. | 7.33 | 27.69 | 58.7 | 57.1 |
| Northern Plains Crater Modification : ESP_043549_2265 ESP_043615_2265 (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 | 45.99 | 220. | -5.7 | -18.9 | 41.7 | 42.7 |
| Gullied Crater in Tempe Terra : ESP_043705_2225 ESP_043771_2225 (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 | 41.98 | 282. | -5.5 | -19.7 | 40.5 | 41.7 |
| Smooth and Knobby Terrain in Lyot Crater Ejecta : ESP_043622_2330 ESP_043754_2330 (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 | 52.55 | 27.4 | -8.9 | -29.3 | 43.9 | 45.5 |
| Cratered Cones within a Flow in Elysium Planitia : ESP_043709_2070 ESP_044408_2070 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.67 | 174. | 0 | -19.6 | 40.0 | 42.5 |
| Central Candor Chasma : ESP_043705_1720 ESP_053766_1720 (Interval in Earth days: 783) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.76 | 287. | 4.77 | -7.87 | 54.6 | 57.0 |
| Boulders on a Landslide: ESP_035831_1760 ESP_036886_1760 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.09 | 324. | 4.56 | -20.6 | 56.9 | 58.6 |
| Inverted Streams in the Aeolis Region: PSP_002424_1765 ESP_019803_1765 (Interval in Earth days: 1354) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.56 | 150. | 0 | -16.3 | 55.7 | 56.6 |
| Floor of East Candor Chasma : ESP_043151_1730 ESP_043428_1730 (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 | -6.84 | 292. | 4.42 | -23.6 | 50.7 | 54.5 |
Page 391 of 877 (8,766 images) | |||||