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.
| Hydrae Cavus: ESP_078625_1720 ESP_079337_1720 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.03 | 298. | -4.1 | 16.02 | 56.8 | 59.5 |
| Partial Icy Fill of Impact Crater onto Graben: ESP_078679_2170 ESP_078824_2170 (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 | 36.46 | 258. | -6.1 | 5.368 | 43.4 | 42.5 |
| Crater in Oxia Planum: ESP_078650_1965 ESP_079151_1965 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.43 | 333. | -9.7 | 12.74 | 46.2 | 46.4 |
| Bright and Round Deposit in Eos Chasma: ESP_078888_1665 ESP_079244_1665 (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 | -13.1 | 319. | -8.5 | 2.452 | 62.1 | 63.3 |
| Layers in Trough in North Polar Layered Deposits: ESP_078635_2660 ESP_078728_2660 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.01 | 327. | 4.56 | -5.38 | 64.3 | 63.8 |
| Terra Cimmeria Dune Monitoring : ESP_078934_1655 ESP_078868_1655 (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 | -14.4 | 142. | 2.23 | 24.21 | 62.5 | 60.7 |
| Sedimentary Layers in Hebes Chasma: ESP_078942_1795 ESP_079298_1795 (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 | -0.55 | 282. | 4.64 | 16.17 | 54.0 | 54.8 |
| Terrain Sample near Jezero Crater: ESP_078844_1980 ESP_078989_1980 (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 | 17.61 | 76.4 | -6.5 | 8.294 | 46.4 | 45.7 |
| Arsia Mons Caldera Southeastern Wall: ESP_078970_1700 ESP_079115_1700 (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 | -10.1 | 239. | -6.7 | 11.71 | 60.5 | 60.2 |
| Alluvial Fans in Kasei Vallis: ESP_078902_2030 ESP_079047_2030 (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 | 22.67 | 293. | -21. | -8.28 | 46.5 | 45.8 |
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