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.
| Layered Mesa near Mawrth Vallis: ESP_076553_2040 ESP_076698_2040 (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 | 23.62 | 336. | -8.0 | 17.59 | 46.1 | 43.0 |
| Landslide Facing East near Aeolis Mensae: ESP_076613_1735 ESP_077655_1735 (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 | -6.41 | 141. | 4.28 | 21.20 | 35.6 | 44.2 |
| 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 |
| Pitted Mounds in Chryse Planitia: ESP_076606_2230 ESP_077292_2230 (Interval in Earth days: 53) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.89 | 326. | -0.9 | -13.6 | 57.6 | 51.0 |
| 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 |
| Fluvial Erosion in Phlegra Montes: ESP_076480_2195 ESP_076823_2195 (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 | 39.32 | 164. | 8.29 | -4.69 | 56.2 | 52.8 |
| Stepped Fan on West Crater Wall of Gale Crater: ESP_076534_1750 ESP_077154_1750 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.00 | 136. | 8.87 | -1.44 | 35.0 | 40.0 |
| Small Delta or Fan: ESP_076526_2030 ESP_077212_2030 (Interval in Earth days: 53) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.52 | 351. | 9.17 | -11.8 | 44.5 | 42.2 |
| Crater on South Polar Layered Deposits: ESP_076642_0915 ESP_059010_0915 (Interval in Earth days: 1374) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.4 | 88.0 | 29.7 | 26.31 | 83.7 | 83.9 |
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