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.
| Pavonis Mons: ESP_039131_1830 ESP_039342_1830 (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 | 2.876 | 244. | 6.87 | -5.46 | 55.0 | 54.2 |
| Seeing Beneath the Surface in Morava Valles: ESP_038798_1665 ESP_039497_1665 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 335. | 0 | -13.8 | 52.6 | 46.3 |
| Candidate ExoMars Landing Site: ESP_038428_1880 ESP_047461_1880 (Interval in Earth days: 704) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.816 | 348. | -1.7 | -18.0 | 59.1 | 55.8 |
| Channels Emanating from Flow Deposit: ESP_038629_1750 ESP_039328_1750 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.03 | 266. | -15. | 5.479 | 56.6 | 49.9 |
| Outflow Channel Landforms in CTX Image: ESP_038490_1430 ESP_064771_1430 (Interval in Earth days: 2048) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.9 | 102. | 0.95 | -18.7 | 56.4 | 60.8 |
| Fractured Mesa in Elysium Planitia: ESP_038659_1815 ESP_038184_1815 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.316 | 168. | -28. | -7.09 | 59.3 | 57.8 |
| Deposits in Libya Montes: ESP_038530_1830 ESP_038398_1830 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.712 | 85.9 | -0.0 | 21.69 | 57.6 | 55.8 |
| Well-Preserved Impact Crater: ESP_038345_1925 ESP_065470_1925 (Interval in Earth days: 2113) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.18 | 93.3 | -5.2 | 4.187 | 60.4 | 61.4 |
| Crater in Isidis Planitia: ESP_038319_1860 ESP_046284_1860 (Interval in Earth days: 620) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.136 | 83.4 | -3.9 | -20.7 | 58.6 | 51.8 |
| Pollack Crater Bedform Changes Near Formation Dubbed White Rock: ESP_038308_1720 ESP_037675_1720 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.01 | 24.9 | 2.08 | -16.1 | 56.0 | 58.8 |
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