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.
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009352_2680 PSP_009618_2680 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.98 | 258. | -6.4 | -18.5 | 63.9 | 65.0 |
| Chain of Vents on Arsia Mons Caldera Floor: PSP_009343_1700 PSP_009976_1700 (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 | -9.69 | 239. | 16.3 | -7.18 | 60.1 | 61.2 |
| Central Structure of Large Crater in Northern Plains: PSP_009332_2360 ESP_018048_2360 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.61 | 171. | 0 | 16.37 | 46.4 | 44.1 |
| Basal Unit and North Polar Layered Deposits in Chasma Boreale Scarp: PSP_009995_2650 PSP_010128_2650 (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 | 85.06 | 0.70 | 19.4 | 5.177 | 65.3 | 66.6 |
| Mound in Small Crater in Utopia Region: PSP_010324_2195 PSP_010390_2195 (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 | 39.39 | 91.8 | -2.9 | -18.2 | 51.0 | 53.1 |
| Hydrated Light-Toned Layers on Crater Floor: PSP_010274_2140 PSP_010696_2140 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.63 | 17.0 | 5.05 | -8.32 | 49.3 | 54.8 |
| Multiple Unconformities in the Upper North Polar Layered Deposits: PSP_010181_2600 PSP_010234_2600 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.74 | 23.4 | -6.9 | -18.7 | 64.6 | 66.2 |
| Eroding Margin of Low Latitude North Polar Layered Deposits: PSP_009938_2640 PSP_010176_2640 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.87 | 139. | 19.6 | 5.57 | 63.3 | 66.3 |
| Possible Intravalley Paleolake in Shalbatana Vallis: PSP_009683_1830 PSP_010316_1830 (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 | 2.989 | 316. | -5.0 | -21.7 | 54.6 | 56.7 |
| Alcove with Bright Rocky Slope Streaks: PSP_009762_1905 PSP_009907_1905 (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 | 10.40 | 318. | -0.3 | 15.26 | 51.2 | 50.3 |
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