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.
| Alluvial Fans in Southeastern Mojave Crater: ESP_039695_1875 ESP_040618_1875 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.214 | 327. | -7.2 | 11.40 | 53.2 | 41.0 |
| Candidate ExoMars Landing Site Near Hypanis Valles: ESP_039735_1920 ESP_040658_1920 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.86 | 314. | 0.25 | 14.90 | 55.2 | 43.0 |
| Gullies and Viscous Flow Feature in Nereidum Montes: ESP_039643_1400 ESP_039709_1400 (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 | -39.4 | 311. | 4.84 | -12.0 | 40.6 | 41.2 |
| Layered Rocks of Ophir Mensa: ESP_039802_1755 ESP_049718_1755 (Interval in Earth days: 773) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.65 | 286. | 8.50 | -1.61 | 44.5 | 31.4 |
| Light-Toned Stratified Materials in Hebes Chasma: ESP_039723_1790 ESP_040211_1790 (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 | -0.57 | 282. | 13.9 | -22.8 | 47.1 | 43.8 |
| Layered Units in Northwest Hellas Region: ESP_039863_1510 ESP_040074_1510 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.8 | 64.7 | 7.12 | -5.58 | 37.4 | 36.5 |
| A Fresh, Shallow Valley in Northern Arabia Terra: ESP_039997_2170 ESP_048792_2170 (Interval in Earth days: 685) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.53 | 0.30 | -17. | 5.074 | 71.1 | 68.1 |
| Fan-Shaped Deposits in Bigbee Crater: ESP_039893_1550 ESP_040394_1550 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 325. | 4.52 | 21.42 | 37.5 | 32.5 |
| Gullies and Bedrock in Nirgal Vallis: ESP_020087_1515 ESP_019810_1515 (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 | -28.2 | 320. | -17. | 5.588 | 62.6 | 63.4 |
| Western Wall of Crater in Kaiser Crater Dune Field: ESP_039245_1325 ESP_039944_1325 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.0 | 18.7 | 4.27 | -19.6 | 47.1 | 42.2 |
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