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.
| Channels Northeast of Hellas Planitia: ESP_093651_1575 ESP_093862_1575 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.5 | 92.4 | 28.0 | 9.301 | 32.2 | 34.8 |
| Chasma Australe Layering: ESP_093559_0940 ESP_093586_0940 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.8 | 95.8 | 28.9 | 15.35 | 70.0 | 71.4 |
| Channel with Mounds near Argyre Planitia: ESP_093643_1420 ESP_093076_1420 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.7 | 314. | 9.56 | 21.56 | 38.7 | 35.7 |
| Lineated Bedrock Block in Protonilus Mensae: ESP_093771_2230 ESP_093982_2230 (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 | 42.77 | 50.1 | -4.9 | -16.6 | 64.0 | 61.6 |
| Gullies in Crater in Terra Cimmeria: ESP_093779_1420 ESP_093344_1420 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.4 | 201. | 5.23 | -10.2 | 40.2 | 38.1 |
| South Polar Layering: ESP_093597_0955 ESP_093637_0955 (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 | -84.4 | 154. | 7.79 | -6.46 | 70.7 | 72.4 |
| Dunes with Erosionally-Resistant Layers in Ross Crater: ESP_093751_1220 ESP_093329_1220 (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 | -57.5 | 251. | -11. | 12.7 | 53.4 | 47.2 |
| Streamlined Shapes in Harmakhis Vallis: ESP_093783_1410 ESP_093216_1410 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.5 | 93.8 | -11. | 10.01 | 41.9 | 36.8 |
| Irregular Cellular Structures around Crater in Southern Mid-Latitudes: ESP_093680_1285 ESP_093614_1285 (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 | -50.9 | 28.5 | -9.1 | 10.29 | 47.8 | 45.9 |
| Crater with Prominent Ridge on Floor with Wall Erosion and Possible Gullies: ESP_093676_1460 ESP_094243_1460 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.8 | 133. | 2.17 | -17.7 | 37.8 | 45.7 |
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