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.
| Gullies on South Rim of Crater in Terra Sirenum Area: PSP_002568_1335 PSP_003201_1335 (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 | -46.4 | 184. | -1.5 | -15.7 | 68.1 | 59.5 |
| Strange Dendritic Relief Features: PSP_001950_2090 PSP_002240_2090 (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 | 28.69 | 126. | -1.5 | 23.36 | 53.0 | 54.0 |
| Sample Main Channel of Athabasca Valles : PSP_002938_1890 PSP_003083_1890 (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 | 8.883 | 155. | 4.35 | 20.17 | 57.0 | 56.2 |
| Layered Deposits within an Unnamed Crater in Arabia Terra: PSP_002100_1840 ESP_060054_1840 (Interval in Earth days: 4515) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.165 | 354. | 0 | -10.2 | 54.3 | 38.9 |
| Tributary of Shalbatana Vallis, As Seen in MOC Image R09-01983: PSP_001930_1835 PSP_002431_1835 (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 | 3.411 | 316. | -0.0 | 24.34 | 54.1 | 53.1 |
| Faulted Layers in Impact Crater in Meridiani Planum : PSP_002733_1880 PSP_002878_1880 (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 | 8.059 | 353. | -6.9 | 8.587 | 57.0 | 56.3 |
| Gullies Possibly Produced by Snow/Ice Melting: PSP_002023_2320 PSP_002524_2320 (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 | 51.75 | 288. | 8.79 | 22.34 | 59.3 | 66.3 |
| Possible Phoenix Lander Landing Site: TRA_000881_2475 TRA_000894_2475 (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 | 67.49 | 130. | -21. | 0 | 54.9 | 53.3 |
| Layered Deposits with Proposed Cross-Bedding: PSP_002023_1755 PSP_002379_1755 (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 | -4.37 | 297. | 2.82 | 12.63 | 55.9 | 54.9 |
| Interior Channel in Parana Valles: PSP_002008_1560 PSP_002285_1560 (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 | -23.9 | 350. | -0.6 | -27.3 | 63.6 | 63.8 |
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