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.
| Channel Entering Northern Mid-Latitude Crater: ESP_088314_2160 ESP_088393_2160 (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 | 35.59 | 6.59 | -6.1 | 19.67 | 43.8 | 41.6 |
| Inverted Channel on Crater Floor near Eden Patera: ESP_088275_2155 ESP_088341_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 | 35.22 | 350. | 5.67 | -13.8 | 42.7 | 44.6 |
| Channel South of Janssen Crater: ESP_088168_1800 ESP_088458_1800 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.118 | 37.6 | -7.2 | 12.15 | 55.4 | 54.8 |
| Grooves and Undercutting in Columbia Valles: ESP_088171_1705 ESP_088316_1705 (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 | -9.60 | 316. | -5.9 | 3.691 | 61.1 | 60.9 |
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_088226_2150 ESP_088661_2150 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.60 | 249. | -5.8 | 17.63 | 43.6 | 42.7 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088230_2400 ESP_088454_2400 (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 | 59.81 | 135. | -4.2 | 14.96 | 47.5 | 46.2 |
| Canyon Wall and Floor in Coprates Chasma: ESP_088290_1655 ESP_088501_1655 (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 | -14.2 | 306. | 8.94 | -6.79 | 63.5 | 64.9 |
| Flow in Tharsis Region: ESP_088055_2035 ESP_088345_2035 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.45 | 241. | -21. | -5.64 | 46.3 | 45.7 |
| Alluvial Fans in Kasei Valles: ESP_088264_2035 ESP_088475_2035 (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 | 23.06 | 294. | -13. | -26.2 | 46.4 | 48.0 |
| Ridges in Nilosyrtis Mensae: ESP_088312_2135 ESP_088246_2135 (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 | 33.36 | 60.4 | 2.84 | 21.93 | 43.1 | 41.2 |
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