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.
| Mesa Stratigraphy at Terby Crater: ESP_083486_1530 ESP_083697_1530 (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 | -26.9 | 73.5 | -4.8 | -22.6 | 44.7 | 43.5 |
| Leveed Feature on North-Facing Valles Marineris Wall Landslide or Glacier: ESP_083425_1710 ESP_084282_1710 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.95 | 295. | 7.89 | -17.7 | 48.8 | 40.7 |
| Troughs Overlying South Polar Layered Deposit: ESP_083661_0930 ESP_083871_0930 (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 | -87.0 | 23.7 | 6.04 | 20.10 | 64.9 | 63.6 |
| Fissure South of Ascraeus Mons: ESP_083321_1780 ESP_083598_1780 (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 | -2.07 | 253. | 1.71 | -24.3 | 53.1 | 52.2 |
| West Hellespontus Complex Dune Field: ESP_083342_1395 ESP_083909_1395 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.1 | 45.1 | 7.14 | -8.63 | 46.1 | 40.8 |
| Gullied Crater Wall in Terra Cimmeria: ESP_083496_1395 ESP_083931_1395 (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 | -39.9 | 161. | 7.83 | 22.1 | 43.9 | 38.2 |
| Landslide on Crater Wall: ESP_083410_1935 ESP_083344_1935 (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 | 13.28 | 341. | 7.82 | 25.40 | 60.0 | 59.1 |
| Linear Ridges Intersecting Valley Topography: ESP_083580_1530 ESP_083514_1530 (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 | -26.5 | 28.7 | -23. | 0.494 | 45.0 | 43.9 |
| USGS Dune Database Entry Number 0894-476: ESP_083314_1320 ESP_083169_1320 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.6 | 89.4 | 17.7 | 5.457 | 47.2 | 50.2 |
| Dune with Seasonally-Persistent Light-Toned Features: ESP_083666_1120 ESP_084378_1120 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -67.8 | 207. | -7.5 | -22.3 | 53.5 | 55.3 |
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