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.
Layering in Argyre Planitia Sinuous Ridge: ESP_012927_1245 ESP_013626_1245 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.1 | 318. | 1.77 | -23.3 | 48.2 | 46.0 |
Layered Bedrock in Northeast Hellas Planitia: ESP_013964_1490 ESP_020267_1490 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.7 | 82.9 | 1.84 | 19.77 | 34.9 | 58.9 |
Gullies: ESP_012722_1400 ESP_012867_1400 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 153. | -6.2 | 7.111 | 47.5 | 44.4 |
Crater Gully Morphology: ESP_013670_1435 ESP_013815_1435 (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 | -36.2 | 190. | 3.34 | 14.46 | 36.5 | 35.3 |
Valleys and Layering along Melas Chasma: ESP_013561_1705 ESP_013983_1705 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.60 | 283. | -0.8 | -18.8 | 40.4 | 37.5 |
Differential Erosion of Light-Toned Stratigraphy in Melas Chasma: ESP_013640_1710 ESP_012928_1710 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.93 | 285. | 8.51 | -10.3 | 39.1 | 48.9 |
Pitted and Fractured Surfaces in Southern Mojave Region: ESP_014034_1870 ESP_014311_1870 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.105 | 327. | 0.98 | -24.4 | 43.1 | 41.9 |
Basal Exposure of South Polar Layered Deposits: ESP_013290_1075 ESP_013092_1075 (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 | -72.2 | 138. | -18. | 5.428 | 55.8 | 55.0 |
Active Geyser Locale: ESP_014083_0945 ESP_014122_0945 (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 | -85.4 | 103. | 8.28 | 22.35 | 69.3 | 68.8 |
Possible Cyclic Bedding in Arabia Terra: ESP_013611_1910 ESP_014033_1910 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.87 | 355. | 0.61 | -17.2 | 50.8 | 46.6 |
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