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.
| Expanded Secondaries on Possible Glacial Unit : ESP_055378_2190 ESP_055444_2190 (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 | 38.91 | 193. | -2.0 | -16.1 | 60.0 | 62.1 |
| Junctions between Wide Channels and Narrow Channels : ESP_055538_1735 ESP_063358_1735 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.67 | 151. | -2.0 | 24.76 | 53.0 | 55.7 |
| Meandering Channels on Western Edge of Acidalia Planitia : ESP_055519_2155 ESP_064038_2155 (Interval in Earth days: 664) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.34 | 304. | 0.23 | -20.2 | 60.3 | 61.3 |
| Holden Crater Rim West of MSL Rover Landing Site: ESP_055268_1535 ESP_055413_1535 (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 | -26.3 | 324. | -1.9 | 17.99 | 59.3 | 56.6 |
| Straight Ridge-Forming Material South of Gill Crater in West Arabia Terra: ESP_055306_1920 ESP_062836_1920 (Interval in Earth days: 587) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.23 | 4.64 | -24. | -4.61 | 54.5 | 49.8 |
| Fan Feature near Memnonia Sulci : ESP_055273_1690 ESP_055761_1690 (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 | -11.0 | 185. | 7.59 | -7.72 | 53.6 | 53.0 |
| Exposed Layers in Medusae Fossae Formation : ESP_055589_1895 ESP_063264_1895 (Interval in Earth days: 598) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.433 | 197. | -3.4 | 8.12 | 53.8 | 51.2 |
| Channel Possibly Sourced from Impact Crater: ESP_055264_1565 ESP_055330_1565 (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 | -23.4 | 72.7 | 6.83 | -13.2 | 57.6 | 58.6 |
| Wrinkle Ridges in West Meridiani Planum : ESP_055412_1795 ESP_059685_1795 (Interval in Earth days: 333) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.57 | 349. | 8.73 | -16.9 | 51.8 | 37.2 |
| Pitted Material on Floor of Well-Preserved Crater in Elysium Planitia : ESP_055314_1985 ESP_055591_1985 (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 | 18.03 | 142. | 8.44 | -8.65 | 52.4 | 56.0 |
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