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.
| 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 |
| Scarp Likely Exposing Polar Layered Deposits in Area Not Well Observed: PSP_005774_0915 ESP_023125_0915 (Interval in Earth days: 1352) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.2 | 212. | 12.6 | 21.16 | 79.7 | 73.9 |
| Aureum Chaos Mineralogical Variability: PSP_006861_1765 ESP_094196_1765 (Interval in Earth days: 6805) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.34 | 332. | 1.00 | -15.8 | 40.0 | 36.6 |
| 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 |
| Possible Exposure of Polar Layered Deposits in Area Not Well Observed: PSP_004882_0880 PSP_004894_0920 (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 | -88.1 | 121. | 11.7 | 11.47 | 68.6 | 67.9 |
| Xanthe Terra Crater: PSP_006598_1780 ESP_033326_1780 (Interval in Earth days: 2083) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.16 | 313. | 2.29 | 24.68 | 37.1 | 37.0 |
| 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 |
| Large Region of Layering in Meridiani Planum: PSP_006227_1810 ESP_011791_1810 (Interval in Earth days: 434) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.126 | 2.68 | 0 | 28.55 | 34.9 | 55.4 |
| Layers Exposed in Central Peak-Pit of Unnamed Crater: PSP_005201_1640 PSP_005913_1640 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.8 | 296. | 5.02 | 22.96 | 33.2 | 32.4 |
| Layers at the Head of Chasma Australe Exposed over 270 Degrees of Azimuth: PSP_004788_0945 PSP_005079_0945 (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 | -85.6 | 95.5 | 0 | -16.3 | 65.3 | 69.7 |
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