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.
Basal Unit and Dunes: PSP_009913_2635 PSP_010019_2635 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.51 | 118. | 8.64 | -5.81 | 63.1 | 64.9 |
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 |
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 Pingos in Gusev Crater: PSP_009385_1655 PSP_009886_1655 (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 | -14.2 | 175. | -18. | 5.226 | 65.1 | 63.0 |
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 |
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 |
Aprons with Channels in Eos Chasma: PSP_009327_1665 PSP_009960_1665 (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 | -13.3 | 317. | 0 | -20.9 | 63.3 | 64.2 |
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 |
Interaction of Cratered Cone and Crater Ejecta: PSP_009906_2225 PSP_010196_2225 (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 | 42.33 | 343. | -7.7 | 14.62 | 48.0 | 48.7 |
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 |
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