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.
Light-Toned Outcrops and Unusual Ridges in Eastern Noctis Labyrinthus: ESP_015922_1720 ESP_016634_1720 (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 | -8.04 | 266. | -0.8 | 20.76 | 44.6 | 50.8 |
Small Valley in Eastern Hellas Planitia: ESP_016100_1385 ESP_016166_1385 (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 | -41.3 | 91.0 | 1.60 | -16.2 | 67.7 | 69.7 |
Ridge Near Olympus Mons: ESP_015976_1945 ESP_016899_1945 (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 | 14.11 | 229. | -5.1 | 12.21 | 39.4 | 42.7 |
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 |
Lineated Valley Floor Material in Terrain North of Arabia Region: ESP_016287_2205 ESP_077488_2205 (Interval in Earth days: 4769) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.04 | 15.5 | -2.8 | 7.652 | 43.1 | 46.5 |
Layered Rocks in Ius Chasma: ESP_016225_1730 ESP_018348_1730 (Interval in Earth days: 166) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.94 | 273. | 0 | -15.1 | 47.4 | 59.4 |
Marte Vallis Streamlined Landforms: ESP_016202_1895 ESP_016835_1895 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.254 | 179. | 5.93 | -8.19 | 40.6 | 45.8 |
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 |
Stratigraphic Relations in MOC Image M00-02426 in Sinus Meridiani: ESP_016169_1790 ESP_019637_1790 (Interval in Earth days: 270) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.77 | 1.73 | 4.18 | -16.4 | 43.8 | 56.0 |
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 |
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