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 Gullies at Multiple Elevations: ESP_067299_1435 ESP_067708_1435 (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 | -36.1 | 227. | -6.6 | 3.913 | 42.9 | 47.4 |
| Layered Deposits on South Wall of West Candor Chasma: ESP_068392_1730 ESP_076832_1730 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.96 | 284. | 21.9 | 0.965 | 43.9 | 37.3 |
| Inverted Channel East of Arabia Terra: ESP_068163_1965 ESP_069021_1965 (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 | 16.13 | 49.6 | -6.4 | -20.8 | 44.3 | 48.6 |
| Channels and Deposits: ESP_068363_2170 ESP_069023_2170 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.68 | 350. | 9.24 | -0.38 | 49.8 | 48.3 |
| Inner Channel in Kasei Valles: ESP_068339_2015 ESP_072111_2015 (Interval in Earth days: 294) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.15 | 287. | 4.31 | -13.1 | 44.6 | 52.5 |
| Terrain in Utopia Planitia: ESP_068121_2145 ESP_072170_2145 (Interval in Earth days: 315) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.10 | 111. | 9.15 | 22.68 | 50.2 | 49.8 |
| Chain of Layered Mounds in Chryse Planitia: ESP_068179_2000 ESP_072663_2000 (Interval in Earth days: 350) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.60 | 332. | -4.3 | 21.53 | 45.1 | 53.6 |
| Streamlined Form in Kasei Valles: ESP_068326_1990 ESP_069474_1990 (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 | 18.78 | 283. | -7.8 | 6.899 | 45.0 | 48.4 |
| Pyramus Fossae: ESP_068149_2310 ESP_077130_2310 (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 | 50.41 | 66.2 | -3.9 | -16.6 | 60.2 | 57.4 |
| 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 |
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