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.
| Gullies on the Northern Crater Slope in Terra Sirenum: ESP_085301_1360 ESP_092685_1360 (Interval in Earth days: 576) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.8 | 194. | 6.97 | -7.35 | 48.5 | 41.4 |
| Cross Cutting in a Crater: ESP_085164_1620 ESP_085718_1620 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.6 | 331. | 7.82 | -8.66 | 35.0 | 41.5 |
| Extensive Boxwork in Terra Sabaea: ESP_084634_1525 ESP_092084_1525 (Interval in Earth days: 580) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.0 | 44.2 | 0.44 | -13.1 | 35.3 | 47.5 |
| Potential Fan Deposit at Head of Mawrth Vallis: ESP_084715_1990 ESP_085005_1990 (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 | 18.91 | 346. | -0.5 | 15.83 | 49.8 | 45.3 |
| Jezero Crater Inlet Valley: ESP_084659_1990 ESP_084949_1990 (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 | 18.65 | 76.0 | -2.9 | 10.01 | 50.4 | 46.1 |
| Gully with Possible Bright Deposit: ESP_084576_1385 ESP_085222_1385 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.2 | 190. | -4.9 | 8.917 | 39.9 | 45.6 |
| Ridge in Lava Flow: ESP_084774_2075 ESP_084550_2075 (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 | 27.39 | 173. | 5.97 | -20.2 | 54.6 | 59.1 |
| Ancient Crust Outcrops at Nectaris Montes: ESP_084519_1650 ESP_084018_1650 (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 | -14.7 | 304. | -17. | -6.83 | 37.1 | 40.8 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084841_0965 ESP_084815_0965 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -83.2 | 171. | 8.58 | -6.10 | 70.6 | 71.2 |
| Channels in Hellas Planitia: ESP_084792_1490 ESP_085570_1490 (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 | -30.8 | 50.7 | -6.9 | 8.445 | 37.3 | 44.7 |
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