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.
| Jezero Crater Outflow Channel: ESP_076879_1980 ESP_076945_1980 (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 | 18.01 | 77.8 | 9.06 | -4.89 | 39.9 | 40.7 |
| Xanthe Dorsa: ESP_076870_2225 ESP_077081_2225 (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 | 42.17 | 320. | -0.1 | 13.43 | 53.8 | 50.7 |
| Channels in Nereidum Montes: ESP_076765_1435 ESP_076132_1435 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.4 | 316. | 7.45 | -16.9 | 48.3 | 41.4 |
| Terrain Sample near Zhurong Rover Landing Site: ESP_076957_2055 ESP_077168_2055 (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 | 25.33 | 109. | -7.7 | 10.93 | 43.9 | 41.5 |
| Gullies on Massif in Argyre Region: ESP_076923_1345 ESP_076224_1345 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.0 | 325. | 7.99 | -7.78 | 56.6 | 46.5 |
| Traverse Ramp in East Coprates Chasma: ESP_076818_1640 ESP_076752_1640 (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 | -15.6 | 306. | 9.47 | 23.67 | 38.7 | 36.8 |
| USGS Dune Database Entry Number 3525-631: ESP_076909_1165 ESP_076988_1165 (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 | -63.1 | 352. | -2.8 | 20.78 | 70.2 | 70.3 |
| Deposits in Aeolis Dorsa: ESP_076995_1735 ESP_076784_1735 (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 | -6.26 | 154. | 19.6 | 0.949 | 37.1 | 36.9 |
| Downwind Hellespontus Regional Barchan Dunes: ESP_076841_1380 ESP_076221_1380 (Interval in Earth days: 48) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.4 | 44.5 | -10. | 12.82 | 53.9 | 43.1 |
| Floor of East Candor Chasma: ESP_077056_1730 ESP_078045_1730 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.86 | 291. | -7.9 | 23.88 | 40.0 | 48.6 |
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