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.
Very Bright and Sun-Facing Gully Deposits in Hale Crater: ESP_014008_1430 ESP_014153_1430 (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 | -36.4 | 322. | -1.9 | 12.21 | 36.7 | 36.3 |
Basal Exposure of South Polar Layered Deposits: ESP_013791_1070 ESP_014134_1070 (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 | -73.0 | 134. | 8.74 | -8.76 | 56.2 | 60.7 |
Recent Gullies in Well-Preserved Crater: ESP_013667_1345 ESP_013944_1345 (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 | -45.2 | 274. | -4.5 | -28.7 | 40.0 | 42.2 |
Crater between Branches of Athabasca Valles: ESP_013460_1900 ESP_013737_1900 (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 | 9.648 | 157. | 4.42 | -23.9 | 51.5 | 50.0 |
Central Structure of Verlaine Crater: ESP_013213_1705 ESP_013635_1705 (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 | -9.25 | 64.1 | -1.2 | -15.7 | 44.8 | 40.8 |
Nili Fossae-NE Syrtis Phyllosilicate-Sulfate Stratigraphy: ESP_013041_1975 ESP_030025_1975 (Interval in Earth days: 1324) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.42 | 76.9 | -3.2 | 12.81 | 61.2 | 60.4 |
Possible Fan Delta: ESP_013531_2140 ESP_022036_2140 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.87 | 17.5 | -8.5 | 21.35 | 68.7 | 68.8 |
Light-Toned Outcrop in Hummock of Iani Chaos: ESP_013717_1790 ESP_013862_1790 (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 | -1.05 | 342. | 5.13 | 18.19 | 42.1 | 39.5 |
Lobate Features in the Charitum Montes: ESP_013165_1275 ESP_013244_1275 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -51.9 | 301. | -4.0 | 20.40 | 45.0 | 42.6 |
Well Preserved 20 Kilometer Diameter Impact Crater: ESP_013684_1455 ESP_020910_1455 (Interval in Earth days: 563) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 168. | -2.8 | 19.71 | 36.4 | 51.7 |
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