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.
| Floor of Uzboi Vallis South of Nirgal Vallis: ESP_042082_1495 ESP_042016_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 | -30.0 | 322. | -4.5 | 16.71 | 53.1 | 50.7 |
| Possible Landing Site for InSight Mission: ESP_042537_1845 ESP_042827_1845 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.215 | 135. | -7.8 | 18.80 | 41.7 | 41.7 |
| Echus Chasma Layered Deposits: ESP_042624_1790 ESP_069316_1790 (Interval in Earth days: 2080) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.04 | 280. | -4.9 | -22.9 | 44.0 | 55.8 |
| Knob near Orcus Patera: ESP_042641_1900 ESP_043142_1900 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.11 | 174. | 3.69 | 21.92 | 39.9 | 41.0 |
| Hellespontus Region Dunes: ESP_042290_1380 ESP_042224_1380 (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 | -41.5 | 45.5 | -5.7 | 14.32 | 64.2 | 62.1 |
| Possible Clays inside Large Crater in Mawrth Vallis: ESP_042147_2035 ESP_024912_2035 (Interval in Earth days: 1343) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.31 | 340. | 9.16 | 26.29 | 38.7 | 35.6 |
| Slope Streak in Noctis Labyrinthus: ESP_042651_1745 ESP_043073_1745 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.44 | 263. | 2.15 | -17.0 | 45.7 | 50.7 |
| Oxia Palus Region: ESP_042134_1985 ESP_053962_1985 (Interval in Earth days: 922) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.04 | 335. | 7.47 | -28.4 | 37.8 | 47.7 |
| Fan on Crater Floor: ESP_042661_1505 ESP_046327_1505 (Interval in Earth days: 286) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.1 | 353. | 3.01 | -13.7 | 60.0 | 61.5 |
| Overlapping Curved Ridges in Crater in CTX Image: ESP_042567_1510 ESP_042633_1510 (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 | -28.5 | 39.8 | 2.71 | -19.4 | 58.5 | 60.6 |
Page 401 of 878 (8,777 images) | |||||