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.
| Transect Across Lower Harmakhis Vallis: ESP_082813_1370 ESP_074413_1370 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.6 | 86.3 | 27.1 | 4.948 | 52.8 | 48.0 |
| Matrona Vallis Channels: ESP_082691_1720 ESP_082902_1720 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.10 | 176. | -2.8 | -23.1 | 56.0 | 56.3 |
| Small Delta or Fan: ESP_082815_1490 ESP_083105_1490 (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 | -30.5 | 32.7 | 3.11 | 21.53 | 53.0 | 47.6 |
| Uphill Facing Scarps and Lobate Deformation on Slope: ESP_082523_2085 ESP_082602_2085 (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 | 28.12 | 78.9 | 6.50 | 29.15 | 67.2 | 65.9 |
| Extra-Crater Sinuous Ridge: ESP_082751_1260 ESP_082817_1260 (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 | -53.7 | 345. | -5.5 | -22.0 | 59.4 | 59.6 |
| Layered Deposits in Liais Crater: ESP_082694_1045 ESP_082681_1045 (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 | -75.4 | 106. | 8.06 | -8.39 | 68.8 | 70.2 |
| Small Scale Channels near Central Pit in Terra Cimmeria: ESP_082521_1440 ESP_083444_1440 (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 | -35.9 | 142. | -6.0 | -22.2 | 58.3 | 46.5 |
| Small Sinuous Ridge at Base of Small Hill in Aeolis Dorsa: ESP_082560_1735 ESP_082771_1735 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.46 | 153. | 0.76 | -24.1 | 56.7 | 57.7 |
| Complex Crater near Streamlined Feature in Bahram Vallis: ESP_082673_1970 ESP_082963_1970 (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 | 16.79 | 304. | 7.69 | 19.83 | 63.0 | 62.5 |
| Lobate Debris Apron in Argyre Region: ESP_082673_1235 ESP_082950_1235 (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 | -56.2 | 314. | 1.62 | -24.9 | 61.2 | 58.6 |
Page 84 of 891 (8,901 images) | |||||