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.
| Oudemans Crater Central Uplift: A Sample of Well-Preserved Layering: PSP_001602_1700 PSP_002446_1700 (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 | -9.91 | 268. | 2.60 | 26.00 | 58.6 | 54.6 |
| Evidence of Multiple Episodes of Gully Formation: PSP_001684_1410 PSP_002027_1410 (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 | -38.8 | 196. | -6.7 | -25.8 | 74.3 | 72.5 |
| Exhumed Layers near Nili Fossae: PSP_002176_2025 PSP_002888_2025 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.23 | 77.0 | 5.71 | 20.84 | 53.8 | 59.1 |
| Mojave Crater Floor and Central Uplift: PSP_002101_1875 PSP_002602_1875 (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 | 7.517 | 327. | 0 | 23.88 | 53.9 | 53.8 |
| Eroding Layers in an Impact Crater: PSP_001503_1645 PSP_002189_1645 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.2 | 89.6 | -0.4 | -26.5 | 61.7 | 61.1 |
| HiRISE Images Mars Pathfinder Site: PSP_001890_1995 PSP_002391_1995 (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 | 19.08 | 326. | -5.8 | 17.05 | 52.4 | 54.4 |
| Exposure of Polar Layered Deposits with Unconformities: PSP_001398_2615 PSP_001780_2615 (Interval in Earth days: 30) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.51 | 47.3 | 0.70 | 25.03 | 65.4 | 69.4 |
| Nothern Residual Cap Crater: PSP_001416_2665 PSP_001470_2665 (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 | 86.52 | 227. | 6.45 | -8.41 | 69.2 | 70.0 |
| Unconformable Deposits in Electric: PSP_001460_1425 PSP_001724_1425 (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 | -36.9 | 185. | 0.70 | -15.0 | 74.5 | 73.4 |
| Layers in a Scarp on Olympus Mons: PSP_001432_2015 PSP_001630_2015 (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 | 21.55 | 222. | -5.8 | -18.4 | 49.2 | 51.5 |
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