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.
Possible Blocky Deposit in Melas Chasma: ESP_013508_1665 ESP_014141_1665 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 289. | 6.08 | -18.0 | 39.2 | 35.6 |
Gullies: ESP_013130_1350 ESP_013631_1350 (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 | -44.5 | 174. | 0.49 | 17.76 | 42.6 | 38.0 |
Light-Toned Material in a Crater in Terra Cimmeria: ESP_013750_1440 ESP_021543_1440 (Interval in Earth days: 608) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.8 | 166. | -2.2 | 19.05 | 36.5 | 43.0 |
Putative Paleolake: ESP_013780_1630 ESP_058667_1630 (Interval in Earth days: 3497) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.7 | 64.7 | 1.57 | -15.2 | 35.8 | 31.8 |
Her Desher Vallis: ESP_013771_1550 ESP_020562_1550 (Interval in Earth days: 529) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 311. | -2.6 | -22.5 | 35.2 | 57.6 |
Crater in the Sirenum Fossae Region: ESP_012918_1450 ESP_013340_1450 (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 | -34.4 | 201. | -7.6 | -20.0 | 44.4 | 40.3 |
Pasteur Crater Mound with Exposed Layers: ESP_013544_1995 ESP_013610_1995 (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 | 19.19 | 24.0 | -4.4 | -23.3 | 57.5 | 57.9 |
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 |
South Polar Layered Deposits Exposed in Bend in Trough Wall: ESP_013830_0940 ESP_014027_0940 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.7 | 172. | 7.85 | 26.64 | 66.5 | 67.5 |
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 |
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