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.
| Well-Preserved Impact Crater: ESP_015905_2235 ESP_016182_2235 (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 | 42.91 | 3.36 | 3.72 | -15.9 | 45.9 | 45.8 |
| Athabasca Valles: ESP_016071_1890 ESP_024708_1890 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.934 | 155. | 7.83 | -16.8 | 39.6 | 38.8 |
| Stranded Lobe of Material with Associated Ridge on Valley Floor: ESP_016238_2180 ESP_017161_2180 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.54 | 273. | -3.4 | 6.789 | 42.5 | 40.5 |
| Gullied Crater Wall: ESP_015950_1395 ESP_016451_1395 (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 | -40.3 | 225. | 4.65 | 25.21 | 64.5 | 70.3 |
| Sinuous Ridge at Contact Between Lineated Valley Fill and Plains Material: ESP_016142_2240 ESP_080745_2240 (Interval in Earth days: 5033) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.67 | 13.6 | -3.2 | 20.12 | 45.2 | 49.8 |
| Cerberus Fossae Cutting Hill: ESP_016229_1895 ESP_016862_1895 (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 | 9.130 | 162. | 4.10 | -9.74 | 40.9 | 46.1 |
| Mounds on Hrad Vallis Mudflow: ESP_016256_2155 ESP_016322_2155 (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 | 35.06 | 142. | -2.8 | -19.2 | 41.7 | 43.0 |
| Juventae Region Mound and Possible Sulfate-Rich Terrain: ESP_015934_1760 ESP_016646_1760 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.74 | 298. | 0 | 21.43 | 42.9 | 48.4 |
| Noachis Terra Sample: ESP_016182_1560 ESP_016815_1560 (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 | -23.5 | 9.41 | 6.53 | -7.78 | 56.2 | 64.3 |
| Central Peak of 70-Kilometer Diameter Impact Crater in Terra Sabaea: ESP_016114_1580 ESP_016470_1580 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.9 | 66.7 | -6.2 | 4.62 | 55.0 | 58.8 |
Page 695 of 877 (8,765 images) | |||||