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.
| Light-Toned Deposits and Possible Fluvial Channels on Floor of Ius Chasma: PSP_010146_1720 PSP_010568_1720 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.96 | 277. | -4.7 | -18.8 | 59.9 | 60.5 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009301_2720 PSP_009528_2680 (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 | 88.07 | 204. | -7.9 | -21.1 | 63.9 | 64.7 |
| Layering in North Polar Layered Deposit Trough: PSP_010261_2595 PSP_010525_2595 (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 | 79.12 | -0.9 | -4.3 | -18.3 | 65.1 | 69.8 |
| Exposure of Polar Layered Deposits on Ridges and Troughs: PSP_009969_2630 PSP_010008_2630 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.92 | 40.8 | -1.7 | 15.24 | 63.7 | 63.3 |
| Exposure of Polar Layered Deposits in Area Not Well Observed: PSP_009359_2715 PSP_009400_2685 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.42 | 42.9 | -12. | -12.2 | 64.8 | 64.2 |
| Central Peak of Crater: PSP_009561_2325 PSP_010260_2325 (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 | 52.40 | 39.8 | 0.54 | -21.0 | 46.6 | 54.9 |
| Small Crater on the North Polar Deposits: PSP_009404_2635 PSP_010221_2635 (Interval in Earth days: 63) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.46 | 346. | -3.3 | 12.01 | 60.1 | 66.3 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010153_2675 PSP_010603_2675 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.58 | 25.7 | -8.4 | -23.4 | 69.2 | 76.0 |
| Debris Flow in Juventae Chasma: PSP_010198_1755 ESP_016290_1755 (Interval in Earth days: 474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.25 | 297. | 0.26 | 22.12 | 57.8 | 45.2 |
| Well-Preserved Crater with Central Peak: PSP_009367_1590 ESP_035357_1590 (Interval in Earth days: 2025) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.6 | 306. | -5.0 | 9.569 | 68.4 | 66.5 |
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