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.
| Crater in Tyrrhena Terra: PSP_006830_1745 ESP_069692_1740 (Interval in Earth days: 4898) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.58 | 99.6 | -3.9 | -21.0 | 40.7 | 61.4 |
| Seasonal Monitoring: PSP_005750_0965 PSP_005921_0965 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -83.6 | 99.6 | -2.1 | 13.97 | 75.7 | 77.5 |
| Fresh Crater: PSP_005517_2240 PSP_005807_2240 (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 | 43.80 | 301. | -0.2 | 20.25 | 65.1 | 59.8 |
| Sinuous Ridge in Argyre Basin: PSP_006730_1235 PSP_007007_1235 (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 | -56.1 | 316. | 7.79 | -14.4 | 69.5 | 75.4 |
| Oblique Impact Exposing Bedrock within A Libya Montes Massif: PSP_005934_1845 ESP_013766_1845 (Interval in Earth days: 611) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.265 | 81.9 | 4.88 | 28.69 | 35.1 | 42.8 |
| 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 |
| Pair of Odd Craters of Hrad Vallis Deposit: PSP_006881_2145 PSP_010375_2145 (Interval in Earth days: 272) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.25 | 141. | 6.74 | -8.95 | 42.8 | 51.5 |
| 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 |
| Light-Toned Layers in Noctis Labyrithus: PSP_006890_1695 ESP_015975_1695 (Interval in Earth days: 708) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.4 | 261. | 2.52 | -22.8 | 42.9 | 48.0 |
| 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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