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.
| Enigmatic Fine-Scale Morphology in Marte Vallis: ESP_027766_2015 ESP_028320_2015 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.21 | 186. | 24.9 | -7.32 | 44.8 | 51.2 |
| Phyllosilicates in Libya Montes Region: ESP_027559_1845 ESP_027836_1845 (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 | 4.654 | 82.1 | -3.6 | -18.9 | 51.7 | 53.2 |
| Secondary Crater Chain in Cerberus Region: ESP_027741_1850 ESP_043433_1850 (Interval in Earth days: 1222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.837 | 153. | 0 | -13.8 | 51.5 | 47.5 |
| North Polar Gypsum Dune Changes: ESP_027436_2615 ESP_027462_2615 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.44 | 180. | -7.2 | 7.495 | 61.5 | 60.9 |
| Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor: ESP_027771_1640 ESP_028470_1640 (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 | -15.7 | 56.6 | 8.78 | -7.44 | 61.0 | 59.4 |
| Dune Migration: ESP_027738_2590 ESP_027646_2590 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.99 | 212. | 7.64 | -8.70 | 62.0 | 62.1 |
| Tilted Block on Olympus Mons Scarp: ESP_027712_2035 ESP_028279_2035 (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 | 23.21 | 223. | -6.3 | 15.88 | 47.0 | 49.0 |
| Northern Residual Cap Crater: ESP_027635_2680 ESP_028042_2680 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.94 | 134. | -17. | -7.27 | 68.2 | 73.0 |
| Possible Future Landing Site in Sabrina Vallis Outlet: ESP_027656_1920 ESP_027168_1920 (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 | 11.87 | 313. | -3.6 | 13.23 | 49.2 | 46.9 |
| Dune Migration: ESP_027412_2600 ESP_027320_2600 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.98 | 110. | 6.47 | -8.84 | 59.6 | 59.8 |
Page 559 of 885 (8,850 images) | |||||