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.
| Hale Crater Rim Complex with Gullies of Both Sides: PSP_006545_1435 PSP_007112_1435 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.9 | 324. | 0 | -12.5 | 52.2 | 62.1 |
| South Polar Layered Deposits Survey: PSP_005302_0880 PSP_005801_0920 (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 | -87.7 | 153. | 6.38 | 18.16 | 73.1 | 78.7 |
| Basal Scarp of South Polar Layered Deposits: PSP_004759_0955 ESP_013897_0955 (Interval in Earth days: 712) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.4 | 156. | 0 | -14.1 | 64.0 | 68.0 |
| Exposure of High-Latitude Polar Layered Deposits Not Well Observed: PSP_005222_0870 PSP_005615_0930 (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 | -87.1 | 191. | 0 | 14.26 | 72.9 | 75.4 |
| Possible Collapse Feature in Impact Crater Ejecta: PSP_005933_2200 ESP_011286_2200 (Interval in Earth days: 417) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.71 | 105. | -6.4 | 11.69 | 56.3 | 62.4 |
| Gullies: PSP_006605_2120 PSP_007251_2120 (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 | 31.46 | 118. | -3.9 | 11.81 | 43.9 | 40.1 |
| Layering in Northwest-Trending Sinuous Ridge: PSP_006875_1255 ESP_011358_1255 (Interval in Earth days: 349) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -54.0 | 317. | 1.97 | -22.9 | 70.7 | 74.6 |
| Aram Chaos Mineralogical Variability: PSP_006808_1840 ESP_085612_1840 (Interval in Earth days: 6141) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.909 | 338. | 0.77 | 21.86 | 37.9 | 35.0 |
| Layered Deposit in Noachis Terra Crater: PSP_005831_1300 PSP_006622_1300 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.7 | 24.3 | -21. | 3.495 | 51.3 | 63.1 |
| Gullies with Extensive Debris Aprons: PSP_006960_1465 ESP_076916_1465 (Interval in Earth days: 5451) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.1 | 152. | 5.24 | 24.98 | 56.8 | 47.6 |
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