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.
Protonilus Mensae Fretted Terrain: ESP_018448_2250 ESP_062913_2250 (Interval in Earth days: 3465) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.85 | 56.1 | -3.9 | 7.677 | 45.1 | 46.8 |
Contact between Two Different Units on Ganges Mensa: ESP_018162_1730 ESP_018663_1730 (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 | -7.15 | 311. | -7.0 | 19.32 | 59.0 | 56.8 |
Central Structure and Layering of a Large Impact Crater: ESP_018263_2230 ESP_018751_2230 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.58 | 67.3 | -5.3 | -27.4 | 43.9 | 49.1 |
Northern Chryse Region: ESP_018346_2125 ESP_018201_2125 (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 | 32.18 | 322. | -3.5 | -15.8 | 44.0 | 44.6 |
Distorted Layers in Noctis Labyrinthus Trough: ESP_018190_1720 ESP_018823_1720 (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 | -8.09 | 265. | 6.34 | -16.3 | 58.7 | 59.5 |
Noctis Labyrinthus Terrain: ESP_018441_1735 ESP_045579_1735 (Interval in Earth days: 2115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.28 | 253. | -2.1 | -25.1 | 58.1 | 55.0 |
Fresh 2-Kilometer Diameter Impact Crater: ESP_018219_2155 ESP_078576_2155 (Interval in Earth days: 4702) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.25 | 189. | -0.7 | 11.46 | 43.1 | 41.8 |
Central Uplift of Impact Crater: ESP_018277_1620 ESP_026202_1620 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.5 | 52.1 | 3.42 | -23.2 | 65.0 | 64.1 |
North Polar Residual Cap: ESP_018357_2630 ESP_018305_2630 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.84 | 354. | 4.67 | -19.6 | 60.0 | 61.3 |
Fresh 3-Kilometer Diameter Crater near Margaritifer Region: ESP_018398_1715 ESP_025690_1715 (Interval in Earth days: 568) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.64 | 347. | 5.56 | -4.83 | 59.0 | 53.7 |
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