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.
| Ancient Fluvial Activity: ESP_076507_1735 ESP_075808_1735 (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 | -6.38 | 153. | 9.25 | 27.49 | 34.8 | 34.9 |
| Two-Color Aeolian Ridges: ESP_076582_1730 ESP_076925_1730 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.92 | 267. | 0 | -15.5 | 35.8 | 39.4 |
| Exposure of South Polar Layered Deposits within Residual Cap: ESP_076503_0915 ESP_076225_0915 (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 | -88.3 | 308. | 22.2 | 29.52 | 82.0 | 76.7 |
| Collapse Terrain near Orson Welles Crater: ESP_076699_1780 ESP_084545_1780 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.83 | 313. | 0.97 | -21.6 | 36.3 | 41.3 |
| Recent Crater: ESP_076364_1170 ESP_082931_1170 (Interval in Earth days: 512) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -62.7 | 107. | -6.3 | 21.22 | 60.8 | 58.0 |
| Valleys and Inverted Channels in Melas Chasma: ESP_076621_1710 ESP_076476_1710 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.11 | 282. | 15.2 | -14.2 | 35.0 | 36.6 |
| Light-Toned Outcrops in Aureum Chaos: ESP_076540_1760 ESP_085520_1760 (Interval in Earth days: 700) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.01 | 333. | 4.68 | -7.04 | 35.4 | 36.7 |
| Cone in Utopia Planitia: ESP_076377_2110 ESP_076443_2110 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.54 | 97.7 | 4.19 | -10.2 | 51.5 | 51.6 |
| Channels in Flaugergues Crater: ESP_076578_1620 ESP_076921_1620 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.9 | 18.1 | 0.55 | -14.7 | 37.6 | 42.6 |
| Channels in Low Latitudes: ESP_076458_1800 ESP_076801_1800 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.10 | 50.8 | 4.86 | -14.8 | 35.8 | 38.0 |
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