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 with Pedestalized Ejecta and Concentric Circles on Floor: ESP_024815_1370 ESP_033373_1370 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.9 | 119. | -3.4 | -21.8 | 66.7 | 64.2 |
| Slope Streak and Reticulate Bedform Monitoring: ESP_024719_2040 ESP_025009_2040 (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 | 23.79 | 212. | -7.7 | 17.03 | 38.5 | 36.7 |
| Polygons North of Banded Terrain in Hellas: ESP_024936_1435 ESP_033494_1435 (Interval in Earth days: 667) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.2 | 55.4 | -3.5 | -23.0 | 63.6 | 61.5 |
| Valleys and Layering in Western Melas Basin: ESP_024888_1705 ESP_028488_1705 (Interval in Earth days: 281) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.64 | 282. | -11. | 11.41 | 46.4 | 55.7 |
| Dunes and Ripples in Valles Marineris: ESP_025297_1730 ESP_025653_1730 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.02 | 275. | 0 | 15.92 | 48.8 | 51.0 |
| Uplifted Jumble of Ancient Bedrock: ESP_025296_1535 ESP_025784_1535 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.3 | 305. | 1.24 | -22.8 | 61.0 | 67.4 |
| What is This Stuff?: ESP_024886_1765 ESP_025308_1765 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.48 | 335. | 4.98 | -8.48 | 42.3 | 47.6 |
| Libya Montes: ESP_024460_1835 ESP_024961_1835 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.674 | 85.6 | 7.39 | 20.84 | 35.8 | 39.0 |
| 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 |
| Well-Preserved 7-Kilometer Impact Crater: ESP_024406_1475 ESP_042076_1475 (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 | -32.1 | 125. | -4.9 | 8.886 | 52.6 | 53.5 |
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