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 and Lobate Flow Feature in Nereidum Montes : ESP_058223_1335 ESP_058790_1335 (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 | -46.0 | 311. | -1.1 | -15.9 | 39.6 | 47.7 |
| Possible Jarosite-Rich Terrain in North Mawrth Vallis : ESP_058182_2060 ESP_058749_2060 (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 | 25.59 | 340. | 4.30 | -14.0 | 52.2 | 45.9 |
| Terrain in Lyot Crater : ESP_058035_2295 ESP_058101_2295 (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 | 48.88 | 30.3 | 8.51 | -7.35 | 73.2 | 73.1 |
| Contrasting Styles of Layering Separated by Unconformity : ESP_058189_1755 ESP_057767_1755 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.57 | 153. | 2.18 | -7.99 | 33.0 | 38.1 |
| Exposed Bedrock in Terrace of 44-Kilometer Diameter Crater in Margaritifer Terra : ESP_057932_1670 ESP_057866_1670 (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 | -12.9 | 331. | -4.7 | 9.629 | 32.8 | 32.4 |
| Exposure of South Polar Layered Deposits : ESP_058100_0915 ESP_057624_0915 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.4 | 122. | 19.8 | 27.08 | 70.4 | 65.0 |
| Possible Mud Volcano : ESP_058214_1555 ESP_075266_1555 (Interval in Earth days: 1329) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.4 | 193. | 4.81 | 16.57 | 30.0 | 36.2 |
| Well-Preserved Ejecta of 20-Kilometer Crater Northeast of Ascraeus Mons : ESP_058040_1995 ESP_058831_1995 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.19 | 259. | -6.3 | 14.41 | 49.8 | 39.1 |
| South Polar Layered Deposits : ESP_057953_0925 ESP_058440_0925 (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 | -87.5 | 179. | 7.63 | 16.48 | 68.7 | 74.3 |
| Eastern Portion of Well-Exposed 6-Kilometer Crater in Ladon Valles : ESP_058209_1620 ESP_057998_1620 (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 | -17.6 | 328. | 7.97 | 22.18 | 29.4 | 29.1 |
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