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.
| Clays and Chlorides in Sirenum Region: ESP_016043_1480 ESP_016188_1480 (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 | -31.6 | 206. | -5.5 | 9.37 | 60.3 | 61.5 |
| Non-Reticulate Bedforms: ESP_016068_1720 ESP_016213_1720 (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 | -8.05 | 240. | -0.9 | 16.85 | 46.3 | 46.8 |
| Gullied Crater Wall: ESP_016191_1415 ESP_026951_1415 (Interval in Earth days: 838) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.1 | 125. | 6.43 | -7.63 | 66.4 | 79.4 |
| Bedrock Bench in Ganges Chasma: ESP_015907_1710 ESP_016830_1710 (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 | -8.94 | 316. | -7.2 | 10.26 | 45.3 | 53.8 |
| Central Peak of an Impact Crater in Terra Sabaea: ESP_016153_1565 ESP_020188_1565 (Interval in Earth days: 314) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 81.0 | 7.63 | -4.44 | 55.4 | 59.1 |
| Layered Material Seen in MOC Image M0807392 in Focas Crater: ESP_016208_2135 ESP_017975_2135 (Interval in Earth days: 138) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.42 | 12.7 | 1.67 | -15.9 | 41.0 | 43.8 |
| 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 |
| Sulfate Layered Stratigraphy in Ophir Region: ESP_015974_1760 ESP_020220_1760 (Interval in Earth days: 331) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.85 | 285. | 4.82 | -15.3 | 43.0 | 56.3 |
| Crater with Rampart-Like Ejecta Exposed in Cross Section: ESP_016080_1745 ESP_025574_1745 (Interval in Earth days: 740) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.30 | 272. | 0 | 11.85 | 45.1 | 49.7 |
| Large Polygons: ESP_016098_1415 ESP_016164_1415 (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 | -38.1 | 144. | 7.55 | -11.8 | 64.9 | 66.9 |
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