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.
| 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 |
| Monitoring Temporal Changes in Danielson Crater: ESP_048621_1885 ESP_048476_1885 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.265 | 352. | 5.74 | -4.42 | 48.6 | 50.6 |
| Spider Topography : ESP_048932_0970 ESP_040453_0970 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.9 | 167. | 5.54 | 20.66 | 62.6 | 65.3 |
| Channel Entering Trough in Terra Sabaea : ESP_048685_1615 ESP_057916_1615 (Interval in Earth days: 719) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.4 | 48.8 | 6.29 | -6.26 | 34.8 | 31.8 |
| Candidate ExoMars Landing Site in Oxia Palus : ESP_048859_1990 ESP_067044_1990 (Interval in Earth days: 1417) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.68 | 335. | -12. | 22.84 | 54.4 | 50.5 |
| 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 |
| Light-Toned Exposed Terrain in Gorgonum Chaos Basin : ESP_048614_1410 ESP_048825_1410 (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 | -38.6 | 190. | 6.04 | -4.19 | 35.4 | 34.9 |
| Tilted Block in Subsided Region South of Orson Welles Crater : ESP_048873_1780 ESP_049651_1780 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.97 | 314. | 2.45 | 12.36 | 39.7 | 31.5 |
| 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 |
| Gullies and Arcuate Ridges in Nereidum Montes : ESP_048623_1385 ESP_049124_1385 (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 | -41.2 | 307. | -23. | -8.80 | 38.3 | 35.9 |
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