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.
| Gullies in Southern Mid-Latitude Crater: ESP_039721_1400 ESP_066147_1400 (Interval in Earth days: 2059) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 343. | -3.3 | 6.732 | 40.4 | 41.9 |
| Candidate Landing Site for 2020 Mission at Sabrina Vallis Delta: ESP_039801_1920 ESP_049717_1920 (Interval in Earth days: 773) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.75 | 313. | -5.0 | -14.4 | 54.7 | 39.5 |
| A Fresh, Shallow Valley in Northern Arabia Terra: ESP_039997_2170 ESP_048792_2170 (Interval in Earth days: 685) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.53 | 0.30 | -17. | 5.074 | 71.1 | 68.1 |
| Fan-Shaped Deposits in Bigbee Crater: ESP_039893_1550 ESP_040394_1550 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 325. | 4.52 | 21.42 | 37.5 | 32.5 |
| Gullies and Bedrock in Nirgal Vallis: ESP_020087_1515 ESP_019810_1515 (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 | -28.2 | 320. | -17. | 5.588 | 62.6 | 63.4 |
| USGS Dune Database Entry Number 2365-596: ESP_039514_1200 ESP_039791_1200 (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 | -59.6 | 236. | 8.44 | -2.94 | 48.3 | 47.3 |
| Candidate Landing Site for 2020 Mission: ESP_039414_1965 ESP_039770_1965 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.47 | 76.6 | 0.89 | 17.44 | 60.9 | 56.8 |
| Small Cone in Hydraotes Chaos: ESP_039550_1805 ESP_039484_1805 (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 | 0.465 | 326. | -10. | 11.74 | 51.3 | 50.4 |
| Impact Crater into Side of Massif: ESP_039230_1545 ESP_039375_1545 (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 | -25.3 | 66.0 | -4.9 | 8.63 | 46.4 | 43.4 |
| Western Rim of Palikir Crater: ESP_039502_1380 ESP_039779_1380 (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 | -41.5 | 202. | -2.2 | -18.4 | 43.1 | 41.5 |
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