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.
| Dune Interaction with Residual Polar Ice: ESP_089075_2590 ESP_088983_2590 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.02 | 81.5 | 19.5 | 4.815 | 58.2 | 58.4 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_088803_1975 ESP_088869_1975 (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 | 17.32 | 336. | 5.29 | -17.1 | 48.0 | 49.9 |
| Hydrae Cavus: ESP_088910_1720 ESP_089055_1720 (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 | -7.72 | 298. | -7.2 | 6.758 | 60.9 | 59.9 |
| Crater Deposits: ESP_088867_2175 ESP_079927_2175 (Interval in Earth days: 696) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.05 | 28.6 | -18. | -8.45 | 46.7 | 46.2 |
| Shearing Structures between Viscous Flow Features: ESP_089078_2200 ESP_089355_2200 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.55 | 24.6 | 5.18 | -17.0 | 45.8 | 49.7 |
| Possible Vent on Volcanic Terrain near Lineated Valley Floor Material: ESP_089020_2110 ESP_089086_2110 (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 | 30.47 | 170. | -7.4 | -24.8 | 46.8 | 48.8 |
| Flow Entering Fretted Terrain Valley: ESP_088814_2165 ESP_088590_2165 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.33 | 31.8 | 16.4 | -18.3 | 43.3 | 45.6 |
| Deposits in Ganges Chasma: ESP_088883_1725 ESP_089094_1725 (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 | -7.29 | 314. | 5.58 | -5.54 | 59.8 | 60.4 |
| Terrain Features around Crater in Arabia Terra: ESP_088875_2215 ESP_088585_2215 (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 | 41.06 | 167. | 2.85 | -12.9 | 44.9 | 45.1 |
| Ismenius Cavus Channel and Fan-Looking Feature: ESP_089052_2140 ESP_089197_2140 (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 | 33.89 | 16.6 | -6.6 | 4.435 | 46.6 | 46.5 |
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