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.
| Landslide and Bedrock: ESP_082633_1520 ESP_091955_1520 (Interval in Earth days: 726) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.4 | 323. | -7.1 | 14.55 | 55.8 | 47.0 |
| Layered Deposits in Burroughs Crater: ESP_082720_1075 ESP_082878_1075 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -72.4 | 117. | 0.60 | 21.39 | 67.4 | 63.2 |
| Fresh Crater East of Huygens Crater: ESP_082761_1670 ESP_083183_1670 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.8 | 64.8 | 4.57 | -24.5 | 54.2 | 52.6 |
| Small Sinuous Ridge at Base of Small Hill in Aeolis Dorsa: ESP_082560_1735 ESP_082771_1735 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.46 | 153. | 0.76 | -24.1 | 56.7 | 57.7 |
| Ridges Associated with Dipping Layers in Reull Vallis: ESP_082839_1390 ESP_083129_1390 (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 | -40.5 | 99.1 | -0.7 | 17.03 | 54.2 | 48.5 |
| Lobate Debris Apron in Argyre Region: ESP_082673_1235 ESP_082950_1235 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -56.2 | 314. | 1.62 | -24.9 | 61.2 | 58.6 |
| Layered Deposits North of Jiji Crater: ESP_082671_1890 ESP_082592_1890 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.138 | 358. | 23.0 | -6.07 | 58.8 | 61.1 |
| Matrona Vallis Channels: ESP_082691_1720 ESP_082902_1720 (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 | -8.10 | 176. | -2.8 | -23.1 | 56.0 | 56.3 |
| Features Southeast of Ostrov Crater: ESP_082804_1520 ESP_083015_1520 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 332. | 5.33 | -10.5 | 52.8 | 51.3 |
| Sample Rim Traverse Hazards at Possible Mars Helicopter Landing Site: ESP_082686_1565 ESP_082897_1565 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.5 | 314. | 5.76 | -14.9 | 54.1 | 53.3 |
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