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.
| Well-Preserved 6-Kilometer Diameter Impact Crater: ESP_017334_2300 ESP_017413_2300 (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 | 49.67 | 230. | -12. | 9.171 | 44.2 | 42.2 |
| Hellas Planitia Terrain: ESP_017644_1420 ESP_025925_1420 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.8 | 56.7 | 5.17 | -12.5 | 79.0 | 76.3 |
| Mini-Chaos in Crater Floor: ESP_017459_1990 ESP_053827_1990 (Interval in Earth days: 2834) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.80 | 61.3 | -4.8 | -27.4 | 44.6 | 46.9 |
| Impact Crater Exposing Stratigraphy in Eos Chasma: ESP_017463_1630 ESP_018241_1630 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.6 | 315. | 4.08 | -7.28 | 63.1 | 65.0 |
| Gullied Crater Wall in Noachis Terra: ESP_017594_1430 ESP_062903_1430 (Interval in Earth days: 3530) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.5 | 341. | 5.18 | -5.34 | 77.9 | 76.3 |
| Central Uplift of an Impact Crater: ESP_017603_1550 ESP_026095_1550 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 94.5 | 2.99 | -24.4 | 69.4 | 68.6 |
| Lava Delta in Eastern Tharsis Region: ESP_017307_2050 ESP_017729_2050 (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 | 24.97 | 249. | 4.76 | -11.9 | 41.7 | 44.1 |
| Layering Exposed in Crater Walls: ESP_017382_1825 ESP_028063_1825 (Interval in Earth days: 833) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.570 | 5.14 | 0.74 | -11.5 | 51.1 | 53.6 |
| Hanging Valley and Terraces in Mangala Valles: ESP_017691_1735 ESP_017902_1735 (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 | -6.18 | 209. | 6.65 | -2.54 | 56.9 | 57.9 |
| Bacolor Crater Gullies: ESP_017681_2135 ESP_017971_2135 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.97 | 118. | -8.0 | 14.61 | 42.4 | 41.1 |
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