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.
| Scallops and Polygons: PSP_001582_2245 PSP_002848_2245 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.35 | 86.4 | 1.92 | 11.02 | 51.4 | 68.6 |
| Light-Toned Layered Material in South Galle Crater : PSP_002866_1280 ESP_064565_1280 (Interval in Earth days: 4808) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -51.8 | 329. | 1.76 | -20.3 | 65.6 | 68.7 |
| Possible Location of Viking Lander 2: PSP_001976_2280 PSP_002055_2280 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.65 | 134. | -1.1 | 21.16 | 57.9 | 57.2 |
| Hale Crater Ejecta in Bond Crater : PSP_002365_1460 PSP_002510_1460 (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 | -33.5 | 324. | 2.23 | 17.11 | 64.6 | 61.9 |
| Ring and Cone Structures atop Rafted Plates in Athabasca Valles : PSP_002648_1880 PSP_003571_1880 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.835 | 153. | -7.9 | 8.478 | 56.7 | 57.0 |
| East Mareotis Tholus: PSP_001364_2160 PSP_001760_2160 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.89 | 274. | 1.07 | -21.4 | 48.0 | 53.8 |
| Landslides on Flat Topography in Elysium Planitia: PSP_001593_1875 PSP_002437_1875 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.187 | 151. | -1.9 | 22.92 | 52.5 | 53.2 |
| Exposure of Polar Layered Deposits Not Well Covered by Mars Global Surveyor: PSP_001342_2680 PSP_001568_2680 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.04 | 62.4 | -6.0 | -13.1 | 70.2 | 72.6 |
| Dendritic Relief Features : PSP_003084_2085 PSP_003229_2085 (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 | 28.30 | 127. | -1.7 | 13.34 | 65.0 | 65.1 |
| Erosion of North Polar Layered Deposits: PSP_001472_2785 PSP_001710_2785 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.23 | 44.7 | 2.28 | 19.61 | 76.1 | 77.4 |
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