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.
| Degradation Morphologies Near Milankovic Crater : ESP_028332_2360 ESP_033857_2360 (Interval in Earth days: 430) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.71 | 213. | 0 | -18.5 | 58.8 | 51.6 |
| Small Tributary Leading into Ares Vallis : ESP_028420_1870 ESP_028842_1870 (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 | 7.277 | 338. | -7.7 | -18.9 | 52.9 | 55.5 |
| Vent and Flow in THEMIS V13163009 : ESP_028585_1910 ESP_028730_1910 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.08 | 153. | -6.5 | 6.504 | 53.1 | 52.8 |
| Fresh Crater on Northern Plains : ESP_028285_2310 ESP_028206_2310 (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 | 50.65 | 56.3 | 4.29 | -18.7 | 55.7 | 56.5 |
| A Pedestal Crater in the Northern Mid-Latitudes: ESP_028598_2230 ESP_035771_2230 (Interval in Earth days: 559) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.65 | 154. | -1.6 | 21.63 | 57.9 | 41.3 |
| Enigmatic Pits and Rises in Noctis Labyrinthus: ESP_028410_1710 ESP_028766_1710 (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 | -8.73 | 253. | -7.1 | 5.899 | 56.9 | 55.2 |
| Getting Luki: ESP_028368_1500 ESP_028724_1500 (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 | -29.5 | 322. | -5.6 | 8.006 | 66.2 | 62.3 |
| Stratigraphy in Crommelin Crater: ESP_017343_1850 ESP_017765_1850 (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 | 4.755 | 349. | 5.41 | -13.3 | 49.4 | 52.1 |
| Fractures in Chryse Planitia: ESP_027959_1990 ESP_028737_1990 (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 | 18.71 | 321. | -5.3 | 7.285 | 48.9 | 53.3 |
| Extensive Outcrops of Rhythmic Stratigraphy in Arabia Region Crater: ESP_028129_1905 ESP_028195_1905 (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 | 10.35 | 1.11 | 4.69 | -15.4 | 50.4 | 52.2 |
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