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.
Jezero Crater: ESP_088707_1985 ESP_088773_1985 (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 | 18.47 | 77.5 | 0.57 | -21.6 | 47.7 | 49.7 |
Monitoring Gullied Crater: ESP_088568_2310 ESP_088634_2310 (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 | 50.71 | 266. | 8.41 | -6.17 | 44.4 | 45.9 |
Alluvial Fan and Light-Toned Deposits in Coprates Catena Trough: ESP_088409_1655 ESP_088119_1655 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.2 | 297. | 5.41 | -13.7 | 63.9 | 64.4 |
Flow Entering Fretted Terrain Valley: ESP_088735_2170 ESP_088669_2170 (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 | 36.59 | 32.1 | -14. | 4.335 | 45.7 | 43.8 |
Gullies on Western Wall of Nier Crater: ESP_088574_2230 ESP_088640_2230 (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 | 42.77 | 105. | -0.5 | -17.0 | 44.0 | 45.8 |
Kasei Valles Alluvial Fans: ESP_088633_2040 ESP_088778_2040 (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 | 23.55 | 298 | -6.4 | 3.817 | 46.5 | 46.1 |
North Polar Layered Deposits Structural Geology in Icy Layers: ESP_088653_2625 ESP_088693_2625 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.34 | 81.4 | 8.18 | -8.30 | 58.5 | 59.6 |
Crater Exposing Structure of Glacial Fill inside Baphyras Catena: ESP_088436_2190 ESP_088647_2190 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.53 | 275. | -8.7 | -18.9 | 44.2 | 45.8 |
Channel Entering Sklodowska Crater: ESP_088512_2130 ESP_088578_2130 (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 | 32.92 | 358. | 15.6 | -3.74 | 42.6 | 44.5 |
Long Section of Exposed Stratigraphy in Eastern Candor Chasma: ESP_088607_1725 ESP_088462_1725 (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 | -7.17 | 291. | 0.37 | -10.5 | 60.0 | 60.6 |
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