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.
| Debris Apron in Phlegra Montes : PSP_002766_2285 ESP_090563_2285 (Interval in Earth days: 6842) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.98 | 165. | 4.28 | -16.3 | 69.9 | 66.8 |
| 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 |
| Impact Crater on North Polar Layered Deposits: PSP_001612_2670 PSP_001956_2670 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.85 | 290. | 0.48 | -11.1 | 72.0 | 77.4 |
| Scalloped Terrain: PSP_001331_2260 PSP_002162_2260 (Interval in Earth days: 64) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.62 | 93.6 | 0 | 19.66 | 49.3 | 58.2 |
| Layers on Floor of West Candor Chasma: PSP_002195_1745 PSP_002406_1745 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.19 | 282. | -5.3 | -11.5 | 56.6 | 56.9 |
| Knobs Near Arrhenius Region : PSP_002478_1365 PSP_003678_1365 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.9 | 120. | 4.1 | -7.1 | 67.4 | 50.5 |
| Athabasca Valles Distributary Channel: PSP_001540_1890 PSP_002371_1890 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.783 | 155. | 16.5 | -3.96 | 50.4 | 55.2 |
| Light-Toned Rock Outcrops in/Near MOC Image R09-00101 North of Sigli Crater: PSP_003090_1600 ESP_037809_1600 (Interval in Earth days: 2705) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.7 | 329. | 1.97 | -25.3 | 54.3 | 61.5 |
| Dark Gullies in Western Argyre Region: PSP_002023_1275 PSP_002102_1275 (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 | -51.9 | 304. | -0.5 | 24.14 | 78.3 | 75.6 |
| Gullies Possibly Produced by Snow/Ice Melting: PSP_002023_2320 PSP_002524_2320 (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 | 51.75 | 288. | 8.79 | 22.34 | 59.3 | 66.3 |
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