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.
| Unnamed, Well-Preserved Crater South of Hypanis Valles: PSP_009393_1890 PSP_010105_1890 (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 | 8.973 | 313. | -3.9 | 13.87 | 51.3 | 51.3 |
| Dark Spot Near Olmpus Mons Volcano: PSP_009502_1980 ESP_015950_1980 (Interval in Earth days: 503) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.62 | 216. | -2.0 | 26.27 | 48.1 | 36.5 |
| Water Bearing Minerals in Noctis Labyrinthus: PSP_009474_1705 PSP_010107_1705 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.28 | 263. | -0.3 | -20.5 | 60.9 | 61.8 |
| Layered Rocks in Northern Hellas Planitia: PSP_008756_1510 PSP_008967_1510 (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 | -28.8 | 69.8 | 7.46 | -14.8 | 72.4 | 74.3 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009263_2675 PSP_009370_2675 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.49 | 182. | -3.5 | -13.3 | 62.9 | 63.2 |
| Transition between Medusae Fossae Formation and Clusters of Aligned Cones: PSP_009175_1810 PSP_009808_1810 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.222 | 145. | -2.2 | -24.0 | 54.7 | 57.1 |
| Tube-Fed Lava Flow Field: PSP_008433_1755 PSP_009501_1755 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.58 | 247. | 7.65 | -15.8 | 54.7 | 59.2 |
| Crater Floor and Central Mound in Gale Crater (MSL): PSP_009505_1755 PSP_009571_1755 (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 | -4.47 | 137. | -7.4 | -28.4 | 58.6 | 60.2 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009243_2675 PSP_009297_2675 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.62 | 13.0 | -5.1 | -13.9 | 62.9 | 63.0 |
| Dark Materials on Block in Olympus Mons Aureole: PSP_008935_1975 ESP_016372_1975 (Interval in Earth days: 580) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.33 | 217. | -8.1 | 5.979 | 47.1 | 40.0 |
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