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.
| Fractured Mounds at the Southern Edge of Elysium Planitia : PSP_002542_1765 PSP_003597_1765 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.25 | 167. | 8.70 | -21.0 | 55.0 | 54.9 |
| 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 | 62.0 |
| 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 | 57.1 |
| Crater and Extensive Field of Secondary Craters Seen in MOC Image R15-02146: PSP_002230_1850 ESP_027890_1850 (Interval in Earth days: 1999) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.727 | 46.1 | -7.8 | 4.118 | 55.2 | 51.4 |
| 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 |
| Kasei Vallis Cataract : PSP_002287_2010 PSP_002788_2010 (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 | 20.76 | 287. | -0.3 | 21.06 | 55.2 | 57.9 |
| 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 |
| Layering in Danielson Crater : PSP_002944_1880 ESP_019835_1880 (Interval in Earth days: 1317) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.951 | 352. | -11. | 10.60 | 58.1 | 52.8 |
| Alluvial Fan in Arabia Terra : PSP_002694_1985 PSP_003195_1985 (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 | 18.24 | 335. | 2.71 | 25.78 | 58.0 | 59.5 |
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