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.
| Dark Lanes in South Polar Residual Cap: ESP_085022_0905 ESP_076186_0905 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.2 | 306. | 26.9 | 29.78 | 77.5 | 76.8 |
| Hillslope Shapes on Holden Crater Rim: ESP_085006_1550 ESP_085151_1550 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 325. | 2.17 | 18.92 | 36.0 | 35.9 |
| Sinuous Flows in Mamers Valles: ESP_085149_2230 ESP_085294_2230 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.88 | 14.2 | -7.1 | 7.44 | 61.7 | 58.8 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084946_1060 ESP_085078_1060 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -73.8 | 175. | -0.6 | -14.4 | 65.2 | 68.1 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_085104_0975 ESP_085012_0975 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.1 | 188. | 7.05 | -7.33 | 73.9 | 73.3 |
| Exhumed Fracture Network: ESP_085266_2080 ESP_085899_2080 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.54 | 62.5 | -9.7 | 6.656 | 49.4 | 42.9 |
| Ice Flow Into Concentric Crater Fill in Nilosyrtis Mensae: ESP_084936_2155 ESP_085292_2155 (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 | 35.23 | 71.5 | -17. | -6.74 | 59.5 | 54.1 |
| Utopia Planitia Mantle Units: ESP_085186_2265 ESP_085331_2265 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.14 | 82.9 | -1.9 | 12.27 | 63.3 | 60.5 |
| Crater: ESP_085139_2030 ESP_085073_2030 (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 | 22.64 | 289. | -7.8 | 11.69 | 47.6 | 47.1 |
| Crater Wall with Potential Chloride Deposit Outcrop: ESP_084905_1470 ESP_085406_1470 (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 | -32.8 | 205. | -5.5 | 26.95 | 38.6 | 42.1 |
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