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.
| Crater in Arabia Terra: ESP_076565_2215 ESP_077053_2215 (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 | 41.35 | 5.62 | -2.6 | 10.14 | 57.2 | 50.7 |
| Inverted Channel and Possible Lake Deposits: ESP_076462_1725 ESP_084242_1725 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.56 | 303. | -5.5 | 29.60 | 35.8 | 38.1 |
| Small Candidate Lake Deposit Downstream of Alluvial Fan: ESP_076629_1675 ESP_076972_1675 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 66.0 | -6.2 | -19.7 | 37.3 | 41.7 |
| Small Delta or Fan: ESP_076539_2150 ESP_077027_2150 (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 | 34.76 | 356. | -6.0 | 7.624 | 53.1 | 47.2 |
| Dipping Layers in Ejecta: ESP_076391_2160 ESP_075824_2160 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.65 | 75.9 | -6.4 | -18.4 | 55.5 | 63.9 |
| Sedimentary Fan in Crater in Terra Cimmeria: ESP_076652_1445 ESP_077140_1445 (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 | -34.9 | 161. | -3.9 | 15.93 | 46.4 | 53.0 |
| Expanded Crater and Scalloped Depressions: ESP_076524_1220 ESP_076880_1220 (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 | -57.4 | 58.6 | -1.2 | 24.75 | 59.2 | 63.9 |
| Youthful Crater in THEMIS V22898007 and at Edge of MOC E11-03928: ESP_076415_1345 ESP_084037_1345 (Interval in Earth days: 594) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.2 | 150. | 5.97 | -6.29 | 48.5 | 41.2 |
| Contact between Wallrock and Interior Layered Deposits in Melas Chasma: ESP_076634_1660 ESP_077676_1660 (Interval in Earth days: 81) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.6 | 289. | -9.2 | 5.336 | 37.7 | 49.1 |
| Aeolian Erosion of Medusa Fossae Formation: ESP_076386_1760 ESP_076241_1760 (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 | -3.93 | 214. | 25.0 | 0.959 | 33.5 | 35.6 |
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