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.
| Western Interior of Tooting Crater : ESP_043721_2035 ESP_043866_2035 (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 | 23.18 | 207. | 2.34 | 18.38 | 40.5 | 39.3 |
| USGS Dune Database Entry Number 0795-196 Changes : ESP_043607_2000 ESP_044385_2000 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.67 | 79.5 | 9.89 | 22.91 | 40.5 | 40.5 |
| Central Candor Chasma : ESP_043705_1720 ESP_053766_1720 (Interval in Earth days: 783) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.76 | 287. | 4.77 | -7.87 | 54.6 | 57.0 |
| Columbia Hills Candidate Landing Site for 2020 Mission : ESP_043551_1655 ESP_043696_1655 (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 | -14.4 | 175. | -24. | -7.34 | 60.0 | 59.6 |
| Boulders on a Landslide: ESP_035831_1760 ESP_036886_1760 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.09 | 324. | 4.56 | -20.6 | 56.9 | 58.6 |
| Inverted Streams in the Aeolis Region: PSP_002424_1765 ESP_019803_1765 (Interval in Earth days: 1354) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.56 | 150. | 0 | -16.3 | 55.7 | 56.6 |
| Infilled Crater with Overlying Secondary Craters in Arcadia Planitia : ESP_043260_2265 ESP_043972_2265 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.21 | 189. | 0.67 | 17.69 | 42.2 | 39.1 |
| InSight Mission Candidate Landing Site : ESP_043183_1845 ESP_043671_1845 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.459 | 135. | 21.3 | -10.5 | 43.7 | 48.4 |
| Intercrater Terrain in Terra Sabaea : ESP_043292_1550 ESP_044413_1550 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.6 | 44.9 | 7.30 | -23.9 | 63.3 | 69.4 |
| Crater with Intersecting Faults in Tempe Terra : ESP_043283_2220 ESP_043560_2220 (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 | 41.94 | 282. | -0.8 | -19.2 | 40.9 | 41.9 |
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