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.
| Potential Fan Deposit in Ritchey Crater with Clays: PSP_007363_1510 PSP_008365_1510 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.4 | 308. | 3.89 | -7.30 | 59.7 | 71.0 |
| Interesting Periglacial Assemblage in Utopia Planitia: PSP_007384_2225 PSP_009467_2225 (Interval in Earth days: 163) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.22 | 86.3 | -1.0 | 14.43 | 44.2 | 43.1 |
| Crater in the Adamas Labyrinthus Region Seen in THEMIS Image V21701005: PSP_007713_2170 PSP_009862_2170 (Interval in Earth days: 167) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.45 | 103. | -4.4 | 10.64 | 41.9 | 45.6 |
| Santa Fe Crater in Chryse Planitia: PSP_007244_1995 ESP_016052_1995 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.19 | 311. | 5.51 | 19.74 | 38.9 | 37.5 |
| Dark Dunes Over Light-Toned Mega-Ripples Seen in MOC Image SP1-26004: PSP_007532_1905 PSP_008679_1905 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.61 | 9.06 | 2.36 | -9.87 | 41.8 | 49.2 |
| Hellas Planitia: PSP_007715_1420 ESP_016022_1420 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.4 | 57.6 | 8.36 | 23.98 | 70.4 | 62.4 |
| Flow-Banded Deformed Terrain of Hellas Basin Floor: PSP_007201_1405 PSP_007491_1405 (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 | -38.9 | 54.9 | -7.0 | 3.906 | 65.3 | 68.9 |
| Upper Section of Northern Olympus Mons Basal Scarp: PSP_007445_2035 PSP_008447_2035 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 223. | -1.4 | -13.8 | 40.1 | 44.4 |
| Fan in Crater in Aeolis Region Associated with Channels: PSP_007883_1800 PSP_009109_1800 (Interval in Earth days: 96) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.22 | 146. | -5.0 | 16.57 | 49.3 | 54.0 |
| Potential Chloride Salts: PSP_007032_1665 ESP_011317_1665 (Interval in Earth days: 334) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.1 | 345. | -3.1 | 26.53 | 46.4 | 56.6 |
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