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.
| Survey Layering and Faulting in Layered Deposits in Candor Chasma: PSP_001377_1685 PSP_001852_1685 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.3 | 286. | 0 | 13.98 | 60.0 | 57.7 |
| Tooting Crater Interior: PSP_001538_2035 PSP_002158_2035 (Interval in Earth days: 48) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.18 | 207. | 23.1 | 11.74 | 47.1 | 53.3 |
| Gullies in Dark Layers in Crater Wall: PSP_002212_1335 PSP_002291_1335 (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 | -46.2 | 184. | -6.7 | 21.92 | 73.0 | 70.0 |
| 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 |
| Potential Lobe of Lahar Flow Front: PSP_002042_2090 PSP_002108_2090 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.85 | 134. | 5.87 | -13.1 | 53.3 | 55.7 |
| Terraced Fan in Memnonia: PSP_001644_1715 PSP_001842_1715 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.60 | 200. | 21.0 | -7.60 | 56.5 | 58.2 |
| Sublimation Processes and Spider Evolution : PSP_002652_0930 PSP_002651_0930 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.9 | 96.5 | 7.08 | 22.50 | 87.8 | 86.4 |
| Debris Apron Material Between Crater Rim and Massif in Promethei Terra: PSP_001938_1405 PSP_002782_1405 (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 | -38.9 | 102. | 2.74 | -20.3 | 71.5 | 63.5 |
| Northern Plains Sample: PSP_001919_2470 PSP_001932_2470 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 66.66 | 247. | -9.9 | 11.07 | 65.6 | 64.2 |
| 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 | 51.3 | 68.6 |
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