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.
Partially-Buried Pre-Existing Crater: PSP_007524_1400 ESP_016108_1400 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 234. | -1.4 | -18.6 | 70.0 | 67.6 |
Crater with Multiple Gully Orientations: PSP_007001_2200 PSP_007937_2200 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.48 | 105. | -8.6 | 6.751 | 45.7 | 41.3 |
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 |
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 |
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 |
Central Peak Region of Canso Crater: PSP_007139_2015 ESP_085442_2015 (Interval in Earth days: 6101) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.34 | 299. | -1.5 | -10.2 | 39.3 | 44.2 |
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 |
Ganges Mensa: PSP_007521_1725 PSP_007877_1725 (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 | -7.23 | 311. | 7.88 | -4.81 | 48.5 | 53.0 |
Possible Sulfates in Ius Chasma: PSP_007509_1720 ESP_050839_1720 (Interval in Earth days: 3376) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.70 | 279. | -2.3 | 13.43 | 49.3 | 36.5 |
Light-Toned Outcrops in North Melas Chasma Wall with Possible Sulfates: PSP_007390_1700 PSP_007680_1700 (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 | -9.78 | 289. | -8.0 | 6.442 | 49.4 | 51.7 |
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