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.
| Light-Toned Outcrops North of Oudemans Crater: ESP_047820_1715 ESP_047886_1715 (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 | -8.59 | 266. | -0.9 | -25.6 | 47.3 | 48.7 |
| Colorful Mounds and Bedrock in Terra Sirenum : ESP_047862_1525 ESP_048152_1525 (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 | -27.0 | 203. | -13. | 9.173 | 44.8 | 39.4 |
| Channels in North Argyre Planitia : ESP_048095_1405 ESP_049018_1405 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.2 | 322. | 1.87 | -16.5 | 41.6 | 35.6 |
| Gully Alcoves Downslope from Each Other : ESP_048113_1425 ESP_048904_1425 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.1 | 190. | -2.9 | 17.32 | 41.3 | 32.5 |
| Lava-Filled Crater in Central Elysium Planitia : ESP_048114_1835 ESP_048470_1835 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.523 | 157. | 2.93 | -9.33 | 50.3 | 48.0 |
| Sinuous Ridge within Valley on Aeolis Planum : ESP_048075_1780 ESP_064756_1780 (Interval in Earth days: 1300) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.84 | 143. | 0 | 23.59 | 48.0 | 55.6 |
| Candidate ExoMars Landing Site in Mawrth Vallis: ESP_047738_2020 ESP_048806_2020 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.94 | 341. | 1.3 | -13.0 | 61.9 | 57.4 |
| Residual South Polar Cap Deposits: ESP_047488_0930 ESP_047503_0930 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.7 | 16.1 | 8.52 | -7.40 | 73.4 | 75.7 |
| Potential Dike Associated with Aromatum Chaos: ESP_047449_1785 ESP_048451_1785 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.30 | 316. | -2.1 | 3.725 | 51.5 | 44.7 |
| Terminal Lobes of Landslide or Large Debris Flow in Melas Chasma: ESP_047450_1685 ESP_048953_1685 (Interval in Earth days: 117) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 290. | -2.4 | 15.23 | 49.3 | 33.6 |
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