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 | 60.1 | 57.7 |
| Gamboa Crater Central Uplift in Acidalia Planitia : PSP_002721_2210 ESP_028724_2210 (Interval in Earth days: 2026) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.77 | 315. | 0.64 | -12.1 | 66.2 | 59.9 |
| 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 | 71.7 | 63.6 |
| 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 | 65.7 | 64.3 |
| Fan Near Aeolis Mensae: PSP_002002_1735 PSP_002279_1735 (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 | -6.24 | 151. | 1.29 | -26.9 | 56.5 | 58.6 |
| Gullies in Dao Valles: PSP_001635_1445 PSP_001978_1445 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.3 | 91.1 | 4.16 | -5.48 | 72.2 | 69.9 |
| 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 | 51.4 | 68.8 |
| Irregular Structures in Huo Hsing Vallis: PSP_002150_2110 PSP_002282_2110 (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 | 30.77 | 65.4 | 8.03 | -27.0 | 54.7 | 59.4 |
| Layering in Crater: PSP_002007_1800 PSP_002429_1800 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.23 | 14.3 | 0 | -13.1 | 55.0 | 56.5 |
| Possible Location of Viking Lander 2: PSP_001976_2280 PSP_002055_2280 (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 | 47.65 | 134. | -1.1 | 21.16 | 57.9 | 57.2 |
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