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.
| Possible Landing Site in Gusev Crater: ESP_035942_1655 ESP_036641_1655 (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 | -14.5 | 175. | 7.90 | -21.5 | 63.0 | 63.8 |
| Exposure of North Polar Layered Deposits: ESP_035949_2660 ESP_035869_2660 (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 | 85.80 | 311. | -8.2 | 6.163 | 62.4 | 61.6 |
| Kasei Valles Lava Surface: ESP_035911_2045 ESP_036056_2045 (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 | 24.40 | 297. | 3.79 | 20.67 | 44.9 | 43.9 |
| Channel between Buttes in CTX Image : ESP_035915_2045 ESP_036614_2045 (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 | 24.25 | 188. | 4.95 | -19.2 | 44.9 | 50.3 |
| Layered Deposits and Dunes in Arabia Terra: ESP_035895_1965 ESP_036172_1965 (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 | 16.07 | 13.1 | 27.0 | 9.517 | 45.3 | 47.7 |
| Elysium Mons Caldera: ESP_035811_2050 ESP_037011_2050 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.62 | 146. | 9.77 | -1.00 | 44.1 | 51.6 |
| Central Structure of Impact Crater: ESP_035765_1645 ESP_037255_1645 (Interval in Earth days: 116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.1 | 328. | -5.6 | 14.37 | 64.3 | 59.6 |
| Possible Chlorite-Bearing Knob in Northwest Hellas Region: ESP_035656_1530 ESP_035801_1530 (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 | -26.8 | 66.3 | -7.3 | 10.43 | 72.3 | 71.2 |
| Karzok Crater Stereo: ESP_035663_1985 ESP_037074_1985 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.37 | 228. | 7.20 | -9.76 | 45.7 | 52.9 |
| Channel in Margaritifer Terra: ESP_035949_1685 ESP_043571_1685 (Interval in Earth days: 594) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.4 | 345. | -7.7 | 18.29 | 62.1 | 55.4 |
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