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.
Perplexing Landforms on Hellas Basin Floor: PSP_007135_1400 ESP_016088_1400 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 56.8 | -4.2 | 16.93 | 64.5 | 65.2 |
Sample South Wall of Olympus Mons Caldera: PSP_007023_1980 PSP_007168_1980 (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 | 17.81 | 226. | -0.2 | 12.29 | 38.7 | 38.1 |
Vertical Exposure of Layering in West Candor Chasma: PSP_007021_1740 PSP_007232_1740 (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 | -5.82 | 283. | 5.28 | -9.86 | 42.3 | 45.8 |
Bright Gully Fans: PSP_007429_2440 PSP_008141_2440 (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 | 63.78 | 292. | 2.14 | -7.16 | 55.0 | 50.5 |
Possible Phoenix Landing Site: PSP_008143_2480 PSP_008301_2480 (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 | 67.96 | 234. | -1.0 | 19.81 | 52.2 | 49.9 |
Faults in Ius Chasma: PSP_008010_1720 PSP_009658_1720 (Interval in Earth days: 129) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.82 | 279. | -4.9 | 7.572 | 54.5 | 59.5 |
Naar Crater: PSP_007046_2030 ESP_025691_2030 (Interval in Earth days: 1453) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 317. | 3.89 | -21.5 | 39.0 | 42.0 |
Crater with Gullies Seen in MOC Image E14-02164: PSP_007250_1415 ESP_015979_1415 (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 | -38.3 | 155. | 5.87 | -13.0 | 64.8 | 64.5 |
Layered Bedrock Exposed in Central Uplift of Crater in Thaumasia Planum: PSP_007113_1595 PSP_007469_1595 (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 | -20.3 | 293. | 4.00 | -7.61 | 50.9 | 56.5 |
Reull Vallis: PSP_007819_1390 PSP_009612_1390 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.6 | 99.6 | -6.4 | 7.67 | 74.7 | 81.0 |
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