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.
| Western Rim of Well-Preserved Impact Crater : ESP_028568_2130 ESP_032893_2130 (Interval in Earth days: 337) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.60 | 253. | 6.82 | -6.33 | 53.8 | 45.3 |
| Layers in Northern Meridiani Planum : ESP_028340_1865 ESP_060001_1865 (Interval in Earth days: 2467) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.308 | 1.62 | 5.28 | -12.5 | 51.8 | 38.1 |
| Ridges and Troughs in Crater East of Hellas Planitia : ESP_028402_1455 ESP_028468_1455 (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 | -34.2 | 114. | 7.97 | -9.94 | 67.6 | 68.2 |
| Rounded Deposit with Light Toned Layers : ESP_028298_2105 ESP_033414_2105 (Interval in Earth days: 399) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.15 | 65.8 | -4.3 | 25.99 | 51.3 | 38.5 |
| Ridge in Eos Chasma : ESP_028342_1635 ESP_034302_1635 (Interval in Earth days: 465) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.5 | 310. | -0.3 | 18.00 | 59.8 | 56.3 |
| Layered Bedrock in Gusev Crater : ESP_028492_1645 ESP_033819_1645 (Interval in Earth days: 415) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.1 | 175. | -6.9 | 16.51 | 59.0 | 49.8 |
| Source Region of Harmakhis Vallis : ESP_028561_1410 ESP_028983_1410 (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 | -38.5 | 94.3 | 7.74 | -8.03 | 68.4 | 64.7 |
| Star and Barchan Dune Changes : ESP_028416_1710 ESP_033519_1710 (Interval in Earth days: 398) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.74 | 89.0 | 2.64 | -25.2 | 56.2 | 45.7 |
| Well-Preserved Impact Crater on Alba Patera : ESP_028410_2170 ESP_028766_2170 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.72 | 247. | -8.1 | 1.304 | 54.1 | 58.0 |
| Layered Deposits in Small Crater in Terra Cimmeria : ESP_028547_1405 ESP_037276_1405 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.9 | 118. | -7.8 | 19.54 | 69.8 | 70.3 |
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