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.
| Jezero Crater Inlet Valley : ESP_068162_1990 ESP_067159_1990 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.66 | 76.6 | -7.4 | 27.38 | 45.0 | 48.8 |
| Crater with Outlet Channel in Southern Highlands: ESP_068258_1480 ESP_073665_1480 (Interval in Earth days: 421) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.5 | 344. | -6.6 | 9.163 | 54.4 | 56.4 |
| Quadruple Exit Breach in Small Fresh Crater: ESP_068267_1440 ESP_073463_1440 (Interval in Earth days: 405) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.8 | 99.7 | -5.3 | 7.646 | 56.9 | 60.0 |
| Layers Exposed in Margins of Two Fans or Deltas: ESP_068189_2015 ESP_069047_2015 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.48 | 57.8 | 14.9 | -4.57 | 44.1 | 47.0 |
| Completely Filled Glacial Crater in Phlegra Montes: ESP_068207_2195 ESP_072480_2195 (Interval in Earth days: 332) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.12 | 284. | 7.99 | 29.27 | 52.2 | 53.5 |
| Valleys in Crater Northeast of Argyre Region: ESP_067704_1500 ESP_073784_1500 (Interval in Earth days: 474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.6 | 334. | 7.13 | 20.86 | 44.0 | 53.7 |
| Crater Floor: ESP_068047_1765 ESP_069182_1765 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.38 | 336. | -7.5 | 2.483 | 42.2 | 53.5 |
| Mounds in Acidalia Planitia: ESP_068074_2280 ESP_068483_2280 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.47 | 312. | -7.6 | 26.38 | 59.5 | 53.0 |
| Channels in Orson Welles Crater: ESP_067797_1790 ESP_075433_1790 (Interval in Earth days: 595) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.14 | 314. | 4.35 | -15.7 | 39.8 | 44.2 |
| Knob on Acidalia Mensa: ESP_067928_2275 ESP_068073_2275 (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 | 47.36 | 336. | -13. | 22.80 | 61.5 | 57.4 |
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