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.
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 |
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 |
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 |
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 |
Dunes in Northern Mid-Latitude Crater: ESP_088469_2410 ESP_088548_2410 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 60.69 | 87.7 | 5.29 | 19.86 | 47.3 | 46.3 |
A Fissure and Channel near Pavonis Mons: ESP_086934_1775 ESP_087435_1775 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.54 | 247. | -7.1 | 24.56 | 49.0 | 51.0 |
Ring-Shaped Mounds in Ceraunius : ESP_086815_2115 ESP_087092_2115 (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 | 31.79 | 249. | 16.7 | -7.37 | 40.6 | 42.5 |
Dune Survey: ESP_088162_2540 ESP_088676_2540 (Interval in Earth days: 41) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.92 | 186. | -0.7 | 14.11 | 53.6 | 53.3 |
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