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.
| Valley Headwalls: ESP_032743_2205 ESP_032888_2205 (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 | 40.04 | 26.1 | 11.6 | 21.84 | 50.5 | 48.2 |
| Rocky Massif in Nilosyrtis Mensae Region: ESP_032781_2090 ESP_032847_2090 (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 | 28.73 | 72.1 | -5.6 | -23.1 | 43.9 | 44.7 |
| Columnar Jointing in Crater Wall: ESP_032741_2040 ESP_032886_2040 (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 | 23.59 | 84.4 | -1.3 | 12.77 | 41.2 | 39.2 |
| Layered Exposures in Southern Argyre Planitia: ESP_032614_1250 ESP_041225_1250 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -54.4 | 323. | -6.5 | 12.04 | 58.9 | 54.9 |
| Incipient Collapse at Cerberus Fossae: ESP_032791_1895 ESP_040835_1895 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.625 | 161. | 0.32 | 21.92 | 35.5 | 39.2 |
| Possible Mars 3 Landing Site: ESP_032737_1345 ESP_032447_1345 (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 | -45.0 | 202. | 5.6 | -16.6 | 53.3 | 49.8 |
| Migrating and Static Sand Ripples on Mars: ESP_032616_1275 ESP_032748_1275 (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 | -52.2 | 267. | 3.02 | -26.0 | 56.8 | 60.7 |
| Lava against an Impact Crater in Elysium Planitia: ESP_018537_1860 ESP_019170_1860 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.980 | 150. | 5.55 | -19.2 | 51.1 | 53.8 |
| Possible Cyclic Bedding within a Crater in Arabia Terra: ESP_018714_1890 ESP_019347_1890 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.969 | 358. | 6.46 | -18.9 | 50.0 | 53.4 |
| South Polar Residual Cap in Late Summer: ESP_032328_0925 ESP_032525_0925 (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 | -87.4 | 265. | 7.19 | 16.55 | 80.8 | 83.2 |
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