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.
| Proposed Site for Future Exploration in Capri Chasma: ESP_085811_1665 ESP_085468_1665 (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 | -13.3 | 312. | -7.7 | 11.52 | 41.0 | 36.0 |
| Impact Crater on Side of Trench Northeast of Alba Fossae: ESP_085918_2370 ESP_086195_2370 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 56.50 | 259. | -0.7 | -23.4 | 60.7 | 58.9 |
| Raised Circular Feature: ESP_085811_2210 ESP_086246_2210 (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 | 40.81 | 305. | -6.0 | 6.055 | 51.8 | 47.1 |
| 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 |
| Ridge-Crater Relationships in Osuga Valles: ESP_085349_1650 ESP_085982_1650 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 321. | -4.2 | 3.855 | 36.6 | 42.7 |
| 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 |
| Northern Terra Cimmeria: ESP_085541_1740 ESP_086319_1740 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.31 | 119. | 3.84 | -8.46 | 36.1 | 44.2 |
| Margin of Athabasca Valles Lava: ESP_085672_1835 ESP_085738_1835 (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 | 3.686 | 142. | 7.88 | -7.30 | 36.3 | 37.7 |
| 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 |
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