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.
| Exposure of High-Latitude Polar Layered Deposits Not Well Observed: PSP_005735_0890 PSP_005721_0910 (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 | -88.7 | 218. | 18.7 | 19.02 | 79.2 | 78.6 |
| Channels or Flow Features with Inverted Topography on Arsia Mons: PSP_005915_1720 ESP_011690_1720 (Interval in Earth days: 450) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.81 | 242. | -5.1 | 8.736 | 33.9 | 56.6 |
| Holden Crater Megabreccia: PSP_006690_1530 PSP_006980_1530 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 325. | -7.5 | 14.55 | 49.3 | 52.4 |
| Gullies in Palikir Crater: PSP_005943_1380 ESP_011428_1380 (Interval in Earth days: 427) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.5 | 202. | 3.28 | -12.4 | 45.9 | 67.3 |
| Breach of Crater Where Valley Begins: PSP_006229_1700 ESP_032245_1700 (Interval in Earth days: 2028) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.78 | 309. | 0 | 16.43 | 35.5 | 31.0 |
| Possible Pingo at the Border Between Fretted Crater Ejecta: PSP_006632_2240 PSP_010337_2240 (Interval in Earth days: 288) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.79 | 98.7 | 1.07 | -21.5 | 50.4 | 53.6 |
| Thermally-Distinct Rays Emanating from Gratteri Crater: PSP_006510_1635 ESP_020922_1635 (Interval in Earth days: 1123) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.3 | 197. | 0 | 27.48 | 40.6 | 49.7 |
| Hummocky Terrain and Polygonal Textures Seen in MOC Image M03-04266: PSP_005827_1260 PSP_006605_1260 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -53.8 | 130. | 7.49 | -8.36 | 52.4 | 66.5 |
| Surface Morphology: PSP_005935_2275 ESP_011855_2275 (Interval in Earth days: 462) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.90 | 49.0 | 0.36 | 19.26 | 61.4 | 73.1 |
| Fine Layers in Central Mound of Large Old Crater: PSP_006187_1915 ESP_011395_1915 (Interval in Earth days: 406) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.35 | 13.5 | 0 | 17.38 | 37.1 | 56.5 |
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