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.
| Utopia Planitia: ESP_067580_2050 ESP_067844_2050 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.87 | 110. | 15.7 | -11.2 | 49.1 | 48.9 |
| Outcrops of Fluvial Deposits in Mesa Flank: ESP_067605_1760 ESP_066510_1760 (Interval in Earth days: 86) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.80 | 152. | 5.52 | -6.48 | 38.9 | 45.6 |
| Searching for Slope Features: ESP_067410_1515 ESP_076853_1515 (Interval in Earth days: 735) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.1 | 76.1 | 5.88 | -23.1 | 40.2 | 47.0 |
| South Polar Residual Cap: ESP_067611_0910 ESP_067467_0910 (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 | -88.9 | 17.0 | 28.7 | 23.99 | 80.6 | 78.8 |
| Well-Preserved Impact Crater: ESP_067461_2035 ESP_077458_2035 (Interval in Earth days: 778) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.43 | 118. | 3.05 | -10.3 | 50.3 | 42.0 |
| Gullies on Mound in Nereidum Montes: ESP_067467_1350 ESP_067876_1350 (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 | -44.5 | 324. | -4.3 | 8.455 | 48.9 | 54.5 |
| Valleys in Tyrrhena Terra: ESP_067594_1635 ESP_073951_1635 (Interval in Earth days: 495) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.2 | 95.0 | -2.2 | 18.88 | 39.7 | 52.0 |
| Gullies Mantling and Glaciers near Dao Vallis: ESP_067581_1440 ESP_067713_1440 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.6 | 91.8 | 4.62 | -9.42 | 45.3 | 48.1 |
| Channel in Wall of Orson Welles Crater: ESP_067322_1790 ESP_075301_1790 (Interval in Earth days: 621) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.88 | 314. | -7.4 | 16.47 | 40.7 | 43.7 |
| Valley-Inverted Channel Transition in Arabia Terra: ESP_067636_1875 ESP_067504_1875 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.578 | 26.2 | -1.2 | 15.33 | 42.0 | 41.2 |
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