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.
Thermally-Distinct Material at Distal Coogoon Valles: ESP_019084_1980 ESP_060437_1980 (Interval in Earth days: 3222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.85 | 336. | -5.5 | 5.547 | 49.5 | 37.7 |
Linear Dunes and Sand Sheets in Herschel Crater: ESP_016916_1655 ESP_017417_1655 (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 | -14.1 | 129. | 5.50 | 22.91 | 58.0 | 60.0 |
Layered Bedrock near Oyama Crater: ESP_018820_2035 ESP_019664_2035 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.40 | 341. | 16.2 | -9.56 | 45.5 | 53.5 |
Glacier?: ESP_018857_2225 ESP_019358_2225 (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 | 42.21 | 50.5 | -6.4 | 8.421 | 47.8 | 51.8 |
Alluvial Fan in Far Western Terra Tyrrhena: ESP_018738_1585 ESP_019160_1585 (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 | -21.4 | 67.0 | 0.22 | -17.5 | 66.6 | 65.9 |
Crosscutting Relationships between Persbo Crater Ejecta and Viscous Flows: ESP_018550_1890 ESP_019262_1890 (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 | 8.989 | 156. | -8.3 | 4.302 | 50.9 | 51.2 |
Steep North-Polar Boundary Scarp Mass Wasting: ESP_018720_2655 ESP_019062_2655 (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 | 85.25 | 158. | -1.9 | 11.92 | 64.7 | 68.1 |
Well-Preserved Impact Crater: ESP_018758_2420 ESP_026538_2420 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 61.71 | 229. | -2.3 | -19.3 | 52.4 | 48.1 |
North Polar Dunes: ESP_018628_2620 ESP_018813_2620 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.95 | 161. | 1.54 | -13.4 | 61.5 | 64.2 |
Exposure of North Polar Layers: ESP_018618_2625 ESP_019079_2625 (Interval in Earth days: 36) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.27 | 73.9 | 0 | 17.13 | 61.7 | 65.7 |
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