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 Arabia Terra: ESP_084912_2215 ESP_076011_2215 (Interval in Earth days: 693) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.02 | 6.54 | -19. | 9.401 | 64.4 | 64.0 |
| Inverted Channels in Noachis Terra: ESP_085294_1610 ESP_085637_1610 (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 | -18.5 | 22.6 | 6.24 | -17.7 | 36.3 | 41.6 |
| Layering Ridge near Surius Vallis: ESP_085033_1255 ESP_085099_1255 (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 | -54.2 | 312. | 8.50 | -5.42 | 51.4 | 53.2 |
| Small Delta or Fan: ESP_085070_2120 ESP_085136_2120 (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 | 31.78 | 11.8 | -1.3 | -18.2 | 54.2 | 54.4 |
| Fresh Infrared-Distinct Crater: ESP_085139_1480 ESP_092958_1480 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.9 | 296. | -2.5 | 16.19 | 40.3 | 35.5 |
| Nirgal Vallis Headwaters: ESP_085046_1530 ESP_085191_1530 (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 | -26.9 | 313. | 8.72 | 25.06 | 36.5 | 36.6 |
| Channels near Huygens Crater: ESP_085240_1615 ESP_085306_1615 (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 | -18.1 | 57.5 | -4.1 | -22.8 | 36.5 | 38.5 |
| Exposure of South Polar Layered Deposits: ESP_085009_0905 ESP_085037_0905 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.5 | 289. | 29.6 | 26.87 | 77.2 | 78.0 |
| Expanded Craters in Southern Highlands: ESP_085080_1285 ESP_085146_1285 (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 | -51.3 | 110. | -2.8 | -17.2 | 50.8 | 52.6 |
| South Polar Residual Cap: ESP_084980_0915 ESP_067508_0915 (Interval in Earth days: 1361) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.3 | 340. | 25.6 | 18.92 | 75.9 | 79.5 |
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