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.
| Young-Looking Gullies on Crater Wall : ESP_048824_1420 ESP_049325_1420 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.8 | 217. | -11. | 12.41 | 35.2 | 33.7 |
| Sediment Lens in Jezero Crater Outlet : ESP_048631_1990 ESP_049343_1990 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.68 | 78.6 | 4.85 | 19.37 | 55.8 | 46.5 |
| Possible Flow Material at Bakhuysen Crater Rim : ESP_048950_1575 ESP_049095_1575 (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 | -22.4 | 14.6 | 0.32 | 15.89 | 32.0 | 29.9 |
| Branched Trough and Pit Feature Associated with Curvilinear Ridge : ESP_048990_1845 ESP_049346_1845 (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 | 4.499 | 358. | 4.92 | 17.76 | 42.0 | 37.0 |
| Dipping Layers Near Reull Vallis : ESP_048986_1415 ESP_058151_1415 (Interval in Earth days: 714) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 113. | 3.21 | 20.49 | 33.8 | 33.2 |
| Western Ejecta and Rays of Istok Crater : ESP_048901_1345 ESP_047754_1345 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.1 | 273. | 16.9 | 0 | 35.7 | 48.1 |
| Isolated Secondary Crater Cluster from Resen Crater in Hesperia Planum : ESP_048973_1520 ESP_049540_1520 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 108. | -7.9 | 4.183 | 32.5 | 31.5 |
| Polar Pit Gullies : ESP_048819_1115 ESP_048687_1115 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -68.5 | 1.53 | -5.7 | 13.54 | 51.4 | 50.0 |
| Folded Layers on Floor of Ius Chasma : ESP_048993_1725 ESP_049138_1725 (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 | -7.56 | 279. | -8.7 | 8.232 | 36.3 | 33.7 |
| Discontinuous Sinuous Ridge within Valley : ESP_048681_1435 ESP_065903_1435 (Interval in Earth days: 1342) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.0 | 160. | 6.13 | 20.21 | 34.3 | 43.0 |
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