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.
Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084628_0935 ESP_084680_0935 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.3 | 250. | 3.97 | 18.69 | 70.7 | 70.3 |
Streamlined Features in Hebrus Valles: ESP_084868_1995 ESP_085567_1995 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.18 | 127. | 9.06 | -7.83 | 47.5 | 42.1 |
Jezero Crater Inlet Valley: ESP_084659_1990 ESP_084949_1990 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.65 | 76.0 | -2.9 | 10.01 | 50.4 | 46.1 |
Gullies on Lobate Flow Feature Basin in Nereidum Montes: ESP_084532_1335 ESP_084967_1335 (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 | -46.1 | 311. | 13.9 | 23.63 | 40.7 | 44.2 |
Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084325_1000 ESP_084562_1000 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.0 | 222. | -6.3 | 13.65 | 62.6 | 64.0 |
Inverted Channel in Noachis Terra: ESP_084385_1585 ESP_084451_1585 (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 | -21.1 | 2.82 | 0.76 | -22.6 | 35.6 | 37.2 |
Possible Well-Exposed Overturned Terrain in Crater near Her Desher Vallis: ESP_084321_1550 ESP_084400_1550 (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 | -24.7 | 311. | -7.1 | 25.15 | 36.4 | 33.4 |
Crater: ESP_084392_1205 ESP_084814_1205 (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 | -59.2 | 177. | 4.76 | -19.8 | 47.9 | 53.6 |
Intersecting Flow Fronts and Channels: ESP_084101_1845 ESP_084391_1845 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.307 | 194. | 1.77 | 11.16 | 48.0 | 43.8 |
Gullied Slope: ESP_084477_1275 ESP_084411_1275 (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 | -51.9 | 16.5 | -8.1 | 8.426 | 44.9 | 43.5 |
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