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.
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 |
Alluvial Fans and Terraced Scarps in Kasei Valles: ESP_088541_2025 ESP_088330_2025 (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 | 22.38 | 291. | -19. | -6.13 | 47.7 | 46.0 |
North Polar Layered Deposits Structural Geology in Icy Layers: ESP_088733_2630 ESP_088562_2630 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.71 | 56.5 | 6.65 | -7.41 | 59.1 | 59.3 |
Ridged Flow-Like Features in Deuteronilus Mensae: ESP_088445_2225 ESP_088511_2225 (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 | 42.33 | 26.8 | 8.67 | -8.24 | 42.8 | 44.5 |
Steep Sandy Slopes in Coprates Chasma: ESP_088554_1660 ESP_088620_1660 (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 | -13.7 | 298. | 11.2 | -14.2 | 63.4 | 65.0 |
Stereo for Kunowsky Crater Dunefield: ESP_088644_2370 ESP_088420_2370 (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 | 56.72 | 350. | 5.32 | -16.7 | 46.6 | 47.9 |
Layering and Contact in Lucus Planum: ESP_088545_1725 ESP_088756_1725 (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 | -7.43 | 184. | -3.0 | -16.9 | 60.3 | 61.4 |
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