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 Wall of Crater in Kaiser Crater Dune Field: ESP_039245_1325 ESP_039944_1325 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.0 | 18.7 | 4.27 | -19.6 | 47.1 | 42.2 |
| Light-Toned Deposits Exposed along Floor of Terra Sabaea Crater: ESP_039269_1550 ESP_039625_1550 (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 | -24.7 | 81.0 | -4.1 | 6.419 | 45.9 | 40.5 |
| Channels and Flows in CTX Image: ESP_039475_1420 ESP_039752_1420 (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 | -37.8 | 217. | 12.0 | -6.91 | 41.8 | 40.1 |
| Nili Patera Dunes: ESP_039599_1890 ESP_039665_1890 (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 | 8.823 | 66.9 | 2.58 | -17.6 | 54.6 | 55.2 |
| Fan Shaped Landforms at Valley Termini in Crater: ESP_039331_1475 ESP_047533_1475 (Interval in Earth days: 639) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.9 | 188. | 0.61 | -24.9 | 44.2 | 50.2 |
| Possible Carbonate in Libya Montes Region: ESP_039216_1835 ESP_039849_1835 (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 | 3.286 | 84.6 | -4.3 | -13.7 | 55.4 | 49.6 |
| Candidate ExoMars Landing Site: ESP_039299_1985 ESP_047501_1985 (Interval in Earth days: 639) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.21 | 335. | 6.94 | -19.6 | 62.4 | 60.7 |
| Debris Apron and Flow Features in Reull Vallis: ESP_039519_1400 ESP_039018_1400 (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 | -39.4 | 96.0 | 13.1 | 0 | 41.4 | 49.3 |
| Bedform Change Detection in Aeolis Mensae: ESP_039596_1720 ESP_041086_1720 (Interval in Earth days: 116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.74 | 151. | -0.0 | 18.23 | 46.1 | 32.4 |
| Well-Preserved Crater South of Hypanis Valles: ESP_039379_1890 ESP_056930_1890 (Interval in Earth days: 1368) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.936 | 313. | -2.4 | 22.35 | 56.9 | 52.3 |
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