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.
| Channel in Terra Cimmeria: ESP_077481_1415 ESP_086355_1415 (Interval in Earth days: 692) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.4 | 217. | 6.91 | 28.75 | 61.4 | 60.7 |
| Aram Chaos: ESP_077107_1820 ESP_077384_1820 (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 | 2.106 | 338. | -5.4 | 6.296 | 38.8 | 39.9 |
| Crater in Arabia Terra: ESP_077251_2150 ESP_077528_2150 (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 | 34.54 | 5.36 | -7.6 | 1.733 | 46.5 | 44.3 |
| Channel-Like Feature: ESP_077076_2250 ESP_077208_2250 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.79 | 97.5 | 7.76 | -9.81 | 52.7 | 52.5 |
| Lower Interior Layered Deposits in Eastern Candor Chasma: ESP_076845_1730 ESP_076911_1730 (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 | -6.94 | 288. | 8.48 | -6.96 | 36.9 | 38.6 |
| Xanthe Dorsa: ESP_076870_2225 ESP_077081_2225 (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 | 42.17 | 320. | -0.1 | 13.43 | 53.8 | 50.7 |
| Ripple Change Detection of Gullied Dunes in Southern Mid-Latitudes: ESP_076842_1275 ESP_076710_1275 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -51.9 | 18.1 | -1.8 | 18.56 | 60.6 | 57.2 |
| Layered Deposits in Impact Crater in Utopia Planitia: ESP_076984_2240 ESP_077960_2240 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.81 | 89.5 | -1.1 | -11.8 | 53.7 | 46.9 |
| Crater in Oxia Planum: ESP_077028_1965 ESP_084900_1965 (Interval in Earth days: 613) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.40 | 333. | -6.3 | 21.74 | 40.2 | 44.5 |
| Streamlined Landforms Adjacent to Shalbatana Vallis: ESP_076989_1895 ESP_076923_1895 (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 | 9.220 | 317. | -0.6 | 13.62 | 38.2 | 37.0 |
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