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.
| Fresh Double-Layered Crater with Possible Ponded Materials: PSP_006945_2350 PSP_007235_2350 (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 | 54.57 | 190. | 1.13 | 12.28 | 54.1 | 50.5 |
| Seasonal Monitoring: PSP_005455_0975 PSP_005547_0975 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.1 | 225. | 1.30 | 15.98 | 69.4 | 69.9 |
| 25-Kilometer Diameter Impact Crater of Hellas Basin Floor: PSP_006766_1355 ESP_020387_1355 (Interval in Earth days: 1062) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.0 | 51.8 | 1.99 | -12.8 | 61.4 | 64.8 |
| Floor of Ares Vallis: PSP_006940_1900 PSP_007876_1900 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.11 | 334. | -1.8 | 20.02 | 38.4 | 42.9 |
| 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 |
| West Mareotis Tholus: PSP_006718_2160 ESP_011557_2160 (Interval in Earth days: 378) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.67 | 271. | 1.41 | -25.3 | 44.9 | 67.7 |
| Fresh Crater on Edge of South Polar Layered Deposits: PSP_005457_0995 PSP_005760_0995 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.5 | 167. | 0.47 | 16.95 | 68.1 | 71.9 |
| Ithaca Region Defrosted: PSP_004666_0945 PSP_004891_0945 (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 | -85.2 | 181. | -0.9 | -18.0 | 64.2 | 67.5 |
| 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 |
| Sulfates in Ius Chasma: PSP_006652_1725 ESP_023398_1725 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.47 | 279. | 0 | 14.79 | 39.1 | 30.7 |
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