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_085555_1005 ESP_085476_1005 (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 | -79.1 | 115. | 5.01 | -4.45 | 79.3 | 78.5 |
| Inverted Channel in Noachis Terra Displaying Morphological Change: ESP_085572_1440 ESP_085506_1440 (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 | -35.7 | 358. | -7.2 | 7.596 | 48.5 | 46.6 |
| Sand Sheet Activity Monitoring: ESP_085641_1275 ESP_085786_1275 (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 | -52.0 | 276. | 3.68 | 24.67 | 60.0 | 61.3 |
| Stepped Features in Tartarus Skopulus: ESP_085684_1800 ESP_085829_1800 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.074 | 175. | 2.52 | 26.97 | 36.6 | 35.2 |
| Dune Monitoring in North Mid-Latitude Bonestell Crater: ESP_085388_2220 ESP_085520_2220 (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 | 41.8 | 329. | -0.3 | -22.8 | 57.2 | 57.0 |
| Baldet Crater Dunes and Sheets: ESP_085345_2030 ESP_086268_2030 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.53 | 65.7 | 1.29 | 20.73 | 44.8 | 38.8 |
| Crater in Acidalia Planitia: ESP_085692_2225 ESP_085349_2225 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.12 | 312. | 0.45 | 14.56 | 53.6 | 57.1 |
| Inverted Channel in Noachis Terra: ESP_085453_1585 ESP_085519_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 | 2.69 | 9.81 | -7.34 | 38.4 | 40.4 |
| Pitted Cones near Crater: ESP_085515_2060 ESP_085449_2060 (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 | 25.75 | 105. | 1.87 | 16.40 | 45.1 | 44.7 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_085475_1065 ESP_085554_1065 (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 | -73.5 | 135. | -4.3 | 10.13 | 73.9 | 74.5 |
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