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.
| Shalbatana Vallis Perched Remnant Fan Deposits: ESP_093089_1805 ESP_092944_1805 (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 | 0.551 | 314. | 26.2 | 15.59 | 41.5 | 44.1 |
| Bedding in Hellas Planitia: ESP_092954_1400 ESP_093033_1400 (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 | -39.8 | 49.5 | -13. | 15.98 | 39.3 | 36.9 |
| Seasonal Monitoring near Dorsa Argentea: ESP_092838_1005 ESP_093036_1005 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -79.3 | 345. | 11.8 | -3.15 | 59.0 | 61.0 |
| Features around Crater near Hellas Planitia: ESP_092807_1375 ESP_092596_1375 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.1 | 102. | 1.17 | 19.52 | 39.6 | 39.7 |
| Dune Field: ESP_093057_1040 ESP_093426_1040 (Interval in Earth days: 29) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -75.7 | 125. | 3.99 | 22.48 | 58.1 | 60.6 |
| Candidate Tianwen-3 Landing Region: ESP_092701_2070 ESP_092912_2070 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.64 | 107. | 5.00 | -11.5 | 64.8 | 63.5 |
| Pie-Like Feature near Amenthes Cavi: ESP_092740_1915 ESP_093386_1915 (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 | 11.45 | 125. | -1.4 | 26.34 | 54.2 | 44.5 |
| Southeast Aeolis Dorsa Inverted Delta Trunk Channel: ESP_093095_1735 ESP_093240_1735 (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 | -6.31 | 153. | -0.0 | 16.51 | 39.9 | 37.3 |
| South Polar Residual Cap Stereo Campaign: ESP_093055_0910 ESP_093014_0910 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.2 | 253. | 23.5 | 26.98 | 67.5 | 66.6 |
| Kasei Valles Flood Grooves and Pedestal Crater: ESP_092892_2035 ESP_092958_2035 (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 | 23.01 | 293. | -3.1 | -24.3 | 60.5 | 61.1 |
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