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.
| Breached Crater Near Marte Vallis : ESP_045634_2035 ESP_045924_2035 (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 | 23.36 | 185. | 6.26 | 26.04 | 44.5 | 45.0 |
| Ophir Chasma Floor : ESP_045459_1755 ESP_045525_1755 (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 | -4.66 | 288. | -4.7 | -27.8 | 52.8 | 54.6 |
| Lava Channel in Eastern Amazonis Planitia : ESP_045765_1995 ESP_046187_1995 (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 | 19.13 | 210. | -0.0 | -18.6 | 46.2 | 51.0 |
| 65-Meter Diameter Crater on North Residual Ice : ESP_045448_2730 ESP_062893_2730 (Interval in Earth days: 1360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.98 | 98.2 | -1.4 | -10.6 | 71.2 | 70.1 |
| Floor of Maja Valles : ESP_045564_1860 ESP_046131_1860 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.044 | 299. | 4.54 | -6.00 | 47.7 | 50.0 |
| Volcanic Flow Features in Southern Elysium Planitia : ESP_045793_1775 ESP_050975_1775 (Interval in Earth days: 404) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.25 | 167. | 6.27 | -8.27 | 50.7 | 37.7 |
| Mesas in Utopia Planitia : ESP_045532_2115 ESP_050925_2115 (Interval in Earth days: 420) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.31 | 90.7 | -6.4 | -26.8 | 44.9 | 42.1 |
| Disrupted Lava Surface in Distal Athabasca Valles : ESP_045543_1870 ESP_053784_1870 (Interval in Earth days: 642) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.989 | 152. | 2.70 | 16.22 | 47.5 | 47.4 |
| Buried Crater in Athabasca Valles Lava : ESP_045530_1855 ESP_046598_1855 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.431 | 148. | -1.4 | 11.56 | 48.3 | 50.4 |
| Small Crater on North Polar Layered Deposits : ESP_045447_2710 ESP_045525_2710 (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 | 89.00 | 126. | -19. | -22.4 | 71.7 | 73.1 |
Page 369 of 878 (8,777 images) | |||||