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.
| Nili Patera : ESP_048671_1890 ESP_092162_1890 (Interval in Earth days: 3389) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.711 | 67.5 | 8.01 | 22.9 | 48.2 | 56.1 |
| Candidate Landing Site for 2020 Mission in Jezero Crater : ESP_048842_1985 ESP_048908_1985 (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 | 18.46 | 77.5 | 7.02 | -14.7 | 53.3 | 53.7 |
| 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 |
| 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 |
| 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 |
| 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 |
| Mass of Viscous Flow Features at Base of Gullied Slope : ESP_048979_1330 ESP_048913_1330 (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 | -46.7 | 307. | -5.8 | 11.28 | 38.1 | 36.9 |
| Crater with Steep Slopes : ESP_048648_1365 ESP_048938_1365 (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 | -43.3 | 344. | -10. | 10.17 | 37.8 | 35.3 |
Page 355 of 891 (8,901 images) | |||||