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.
| Massif in Reull Vallis: ESP_024051_1365 ESP_024407_1365 (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 | -43.2 | 97.0 | 7.01 | 22.35 | 53.8 | 59.0 |
| Alluvial Fans and Hanging Valley Morphology in Kasei Valles: ESP_024215_2030 ESP_024637_2030 (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 | 22.69 | 291. | 8.75 | -2.72 | 37.8 | 37.9 |
| Well-Preserved 8 Kilometer Crater: ESP_024080_1340 ESP_032928_1340 (Interval in Earth days: 690) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.4 | 25.7 | 6.66 | 20.83 | 55.9 | 56.0 |
| Prominent Channel Form on Tyrrhena Patera: ESP_024222_1590 ESP_024723_1590 (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 | -20.9 | 107. | -7.9 | 15.92 | 43.1 | 48.9 |
| Fretted Terrains: ESP_024103_1370 ESP_024248_1370 (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 | -42.6 | 118. | -2.2 | 13.74 | 54.7 | 56.3 |
| Banded Landforms in Gullied Kampot Crater: ESP_024254_1380 ESP_041133_1380 (Interval in Earth days: 1315) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.7 | 314. | 13.2 | -3.17 | 55.8 | 45.7 |
| Cerberus Fossae Streak and Bedform Changes: ESP_024075_1930 ESP_024563_1930 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.74 | 154. | 3.78 | -23.4 | 35.2 | 38.4 |
| Mantle Removal around Gully Fan: ESP_024027_1345 ESP_024304_1345 (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 | -45.4 | 33.9 | -5.9 | -21.5 | 55.7 | 61.3 |
| Proctor Crater Dune Changes: ESP_024291_1320 ESP_024370_1320 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.6 | 30.3 | -29. | -0.98 | 63.3 | 62.9 |
| Candor Chasma Dune Changes: ESP_024255_1750 ESP_024110_1750 (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 | -4.79 | 283. | 0.86 | -19.4 | 36.3 | 36.6 |
Page 607 of 885 (8,850 images) | |||||