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.
| Rocky Outcrops Northwest of Elysium Region: ESP_024537_2080 ESP_072314_2080 (Interval in Earth days: 3723) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.64 | 140. | 2.98 | 22.18 | 39.0 | 50.8 |
| Large Impact Crater Northwest of Lyot Crater: ESP_024370_2445 ESP_024291_2445 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 63.94 | 10.5 | 13.3 | -2.50 | 62.1 | 64.0 |
| Channel in Lava Flow: ESP_024530_1570 ESP_042200_1570 (Interval in Earth days: 1377) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.6 | 338. | -5.9 | 11.68 | 48.5 | 49.2 |
| Faulted Layers in Becquerel Crater: ESP_024582_2015 ESP_024503_2015 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.36 | 352. | 10.4 | -21.2 | 36.6 | 39.3 |
| Valley Termini on Western Hecates Tholus: ESP_024418_2125 ESP_024273_2125 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.42 | 149. | 1.81 | -15.4 | 41.6 | 43.8 |
| Monitor Small Fresh Crater Slopes: ESP_024329_1930 ESP_024474_1930 (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 | 12.64 | 61.8 | -5.4 | 12.10 | 36.1 | 35.1 |
| Faults in Claritas Rupes: ESP_024388_1560 ESP_024243_1560 (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 | -23.7 | 254. | 4.57 | -16.8 | 46.4 | 45.6 |
| Layered Material and Proposed Site for Future Exploration: ESP_024553_1500 ESP_024843_1500 (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 | -29.8 | 71.8 | -7.0 | 15.99 | 53.5 | 56.6 |
| Inverted Channels and Fans on Southwest Rim of Kaiser Crater: ESP_024410_1325 ESP_024476_1325 (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 | -47.1 | 17.4 | 7.20 | -10.7 | 62.8 | 64.9 |
| Layers on Northern Rim of Hellas Basin: ESP_024408_1500 ESP_031911_1500 (Interval in Earth days: 585) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.4 | 70.8 | -7.5 | 5.233 | 51.0 | 33.6 |
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