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.
| Meridiani Planum : ESP_044718_1780 ESP_046274_1780 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.19 | 354. | 2.37 | 19.53 | 52.6 | 49.7 |
| Unusual Crater in Amazonis Planitia : ESP_044855_2090 ESP_044921_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 | 28.72 | 210. | 3.03 | -12.8 | 41.0 | 42.5 |
| Atypical Landform among Dunes in Polar Erg : ESP_044917_2575 ESP_044864_2575 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.54 | 307. | -7.0 | 8.026 | 57.6 | 56.4 |
| Possible Gray Hematite in Capri Chasma : ESP_044891_1665 ESP_045313_1665 (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 | -13.3 | 313. | 1.73 | 14.11 | 59.2 | 56.8 |
| Eos Chasma : ESP_044759_1660 ESP_045603_1660 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 316. | -5.6 | 4.319 | 60.3 | 56.7 |
| 60-M Diameter Crater on North Polar Layered Deposits : ESP_044872_2655 ESP_044728_2655 (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 | 85.64 | 58.4 | 5.53 | -14.6 | 62.4 | 62.3 |
| Cross-Cutting Channels in Olympica Fossae : ESP_044735_2050 ESP_044880_2050 (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 | 24.88 | 246. | 5.00 | 24.41 | 41.1 | 39.7 |
| Channels on Alba Mons : ESP_044814_2270 ESP_045157_2270 (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 | 46.47 | 246. | 6.41 | -14.1 | 41.6 | 45.4 |
| Possible Phyllosilicates Associated with Crater South of Aurorae Chaos : ESP_044930_1690 ESP_062877_1690 (Interval in Earth days: 1398) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.8 | 328. | 2.29 | -7.56 | 57.4 | 60.6 |
| Fractures and Exposed Bedrock in Lyot Crater : ESP_044756_2300 ESP_045099_2300 (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 | 49.56 | 28.7 | 8.24 | -10.8 | 42.1 | 45.7 |
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