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.
| Mound in Utopia Planitia : ESP_050529_2095 ESP_055144_2095 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.33 | 99.8 | 2.02 | 25.24 | 41.5 | 51.4 |
| Eastern Floor of Roddy Crater: ESP_050508_1580 ESP_050086_1580 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.7 | 320. | -12. | 15.28 | 40.5 | 33.2 |
| Candidate ExoMars Landing Site in Oxia Palus Region : ESP_050705_1985 ESP_068456_1985 (Interval in Earth days: 1383) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.49 | 335. | 7.05 | 20.97 | 35.2 | 42.8 |
| Slope Monitoring : ESP_050704_1700 ESP_050849_1700 (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 | -9.87 | 6.85 | 1.28 | 14.85 | 36.7 | 37.4 |
| Gullies and Fissures : ESP_050592_1365 ESP_050658_1365 (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 | -43.1 | 190. | -6.6 | -24.4 | 55.3 | 57.5 |
| USGS Dune Database Entry Number 1379-672 Changes: ESP_050515_1125 ESP_050502_1125 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -67.2 | 137. | -1.2 | -25.3 | 72.9 | 74.0 |
| Southwest Arabia Terra Landforms : ESP_050744_1840 ESP_051812_1840 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.780 | 353. | -7.8 | 17.77 | 34.6 | 41.4 |
| Well-Preserved Crater : ESP_050586_1335 ESP_050863_1335 (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 | -46.3 | 353. | 2.21 | -22.7 | 57.1 | 63.2 |
| Northern Plains Ridge : ESP_050846_2305 ESP_050978_2305 (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 | 50.20 | 82.1 | -2.9 | -27.9 | 52.1 | 52.4 |
| Candidate Human Exploration Zone of Maja Valles Entry into Chryse Planitia : ESP_050706_1980 ESP_050416_1980 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.84 | 306. | 28.6 | 8.519 | 33.1 | 35.9 |
Page 320 of 878 (8,777 images) | |||||