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.
| Mawrth Region Crater with Possible Sedimentary Features: ESP_025123_2045 ESP_026811_2045 (Interval in Earth days: 131) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.24 | 340. | 12.4 | -19.9 | 37.4 | 44.7 |
| Scalloped Depressions in Utopia Planitia: ESP_025277_2275 ESP_025620_2275 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.06 | 93.7 | 3.37 | -24.0 | 43.5 | 44.5 |
| Flow Ridges in Nilosyrtis: ESP_025291_2100 ESP_027823_2100 (Interval in Earth days: 197) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.75 | 74.5 | 1.68 | -23.1 | 38.8 | 48.8 |
| Channels in Northern Arabia Region: ESP_025122_2215 ESP_026177_2215 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.18 | 6.08 | 6.88 | -8.44 | 41.6 | 41.2 |
| Reticulate Bedform and Recent Impact Crater: ESP_025152_1945 ESP_025007_1945 (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 | 14.48 | 268. | 28.3 | 15.12 | 36.7 | 37.2 |
| Light-Toned Layering along Floor of Small Trough Near Juventae Chasma: ESP_025072_1730 ESP_028171_1730 (Interval in Earth days: 241) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.83 | 298. | 0 | -14.8 | 46.3 | 57.2 |
| Dunes: ESP_025330_1730 ESP_025475_1730 (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 | -6.93 | 93.9 | 8.60 | 25.68 | 48.5 | 48.7 |
| Well-Preserved Crater Near Alba Patera: ESP_025219_2270 ESP_025285_2270 (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 | 46.56 | 238. | -9.6 | -22.5 | 44.5 | 45.3 |
| Western Hecates Tholus Valleys: ESP_025275_2125 ESP_024985_2125 (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 | 32.22 | 149. | 20.2 | -5.23 | 37.6 | 40.0 |
| Well-Preserved 8-Kilometer Impact Crater with Central Peak: ESP_025295_2090 ESP_025994_2090 (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 | 28.72 | 325. | 6.64 | -19.1 | 38.4 | 41.8 |
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