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.
Central Peak of Large 40-Kilometer Diameter Crater: PSP_007592_1995 ESP_045595_1995 (Interval in Earth days: 2961) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.25 | 169. | -0.9 | 19.06 | 40.8 | 43.5 |
Deposits in Kasei Valles: PSP_007970_2015 ESP_033551_2015 (Interval in Earth days: 1993) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.06 | 287. | -0.6 | 17.86 | 42.0 | 36.8 |
Knobs and Cones in Acidalia Planitia: PSP_007506_2220 ESP_051759_2220 (Interval in Earth days: 3448) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.57 | 354. | 3.16 | 20.33 | 43.2 | 38.9 |
Well-Exposed Central Uplift in Unnamed Crater: PSP_007252_1615 ESP_015981_1615 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.4 | 98.7 | -0.9 | -22.0 | 52.1 | 52.3 |
Western Half of Central Peak of Large Well-Preserved Crater: PSP_007857_1475 PSP_010006_1475 (Interval in Earth days: 168) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.0 | 140. | -6.7 | 19.27 | 68.9 | 72.7 |
Southern Highlands High Thermal Inertia and Spectrally-Distinct Materials: PSP_007254_1565 PSP_007610_1565 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.1 | 43.9 | 8.62 | -4.71 | 54.4 | 59.9 |
Topographically-Deflected Ejecta in Chryse Planitia: PSP_007916_2010 ESP_016078_2010 (Interval in Earth days: 636) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.91 | 322. | 0.50 | 15.41 | 41.8 | 38.0 |
Mound and Trough System in Arcadia Planitia: PSP_007684_2230 PSP_007895_2230 (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 | 42.81 | 173. | 4.97 | -7.90 | 42.8 | 43.4 |
Well-Preserved Gullied Impact Crater in Utopia Planitia: PSP_007726_2165 PSP_008148_2165 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.35 | 107. | 6.41 | -20.9 | 41.0 | 43.3 |
Layered Terrain on Hellas Basin Floor: PSP_007399_1385 ESP_016563_1385 (Interval in Earth days: 715) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.4 | 48.4 | -6.2 | 22.94 | 69.9 | 72.6 |
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