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.
| Fine Layer Deformation in Lobate Debris Apron: ESP_088932_2270 ESP_089275_2270 (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 | 46.44 | 49.8 | 2.69 | -29.9 | 45.8 | 51.3 |
| Possible Skylight in Elysium Planitia: ESP_089152_1885 ESP_089297_1885 (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 | 8.505 | 168. | 1.84 | 15.89 | 52.2 | 51.3 |
| Kasei Valles Flood Grooves: ESP_089015_2055 ESP_089305_2055 (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 | 25.40 | 307. | -6.3 | 17.83 | 47.4 | 46.6 |
| Deposits in Ganges Chasma: ESP_088883_1725 ESP_089094_1725 (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 | -7.29 | 314. | 5.58 | -5.54 | 59.8 | 60.4 |
| Hydrae Cavus: ESP_088910_1720 ESP_089055_1720 (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 | -7.72 | 298. | -7.2 | 6.758 | 60.9 | 59.9 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_089014_1995 ESP_089080_1995 (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 | 19.15 | 335. | 2.69 | -18.5 | 48.1 | 50.1 |
| Dune Interaction with Residual Polar Ice: ESP_088917_2590 ESP_088970_2590 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.89 | 82.0 | 8.16 | -5.86 | 57.7 | 58.9 |
| Antoniadi Crater Fluvial Features: ESP_088945_2015 ESP_089222_2015 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.18 | 58.3 | 7.36 | -21.9 | 47.0 | 50.4 |
| Streamlined Feature in Elaver Vallis: ESP_089015_1710 ESP_089160_1710 (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 | -9.05 | 311. | 5.33 | 19.12 | 60.8 | 59.7 |
| Mesa with Cone on Top: ESP_089062_2055 ESP_089774_2055 (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 | 25.06 | 104. | -1.2 | 15.52 | 47.2 | 49.8 |
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