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.
| Fresh Shallow Valleys in Electris Region: ESP_032580_1350 ESP_032725_1350 (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 | -44.5 | 169. | -3.5 | 8.663 | 50.8 | 52.6 |
| Streamlined Forms in Athabasca Valles: ESP_032699_1875 ESP_033200_1875 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.582 | 153. | -6.5 | 8.57 | 35.5 | 35.7 |
| Possible Hydrated Silicates in Acidalia Planitia: ESP_032850_2200 ESP_033641_2200 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.91 | 347. | -6.6 | 21.87 | 50.4 | 41.9 |
| Streamlined Landforms in THEMIS Image V27359007: ESP_032745_1415 ESP_032811_1415 (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 | -38.3 | 341. | 19.2 | 0.849 | 47.9 | 50.1 |
| Layered Materials on Northeast Hellas Region Rim: ESP_032636_1525 ESP_032781_1525 (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 | -27.3 | 78.1 | -7.4 | 7.913 | 41.3 | 42.4 |
| Gullied Crater: ESP_032883_1400 ESP_033173_1400 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 175. | -2.3 | 16.04 | 52.4 | 56.3 |
| Viscous Flow: ESP_032875_2195 ESP_033165_2195 (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 | 39.34 | 24.7 | -7.0 | 8.757 | 49.7 | 45.9 |
| Thermokarst: ESP_032872_1405 ESP_040837_1405 (Interval in Earth days: 621) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.2 | 116. | -3.2 | -16.8 | 52.1 | 41.5 |
| Very Well-Preserved Crater in Ares Vallis: ESP_032521_1955 ESP_032943_1955 (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 | 15.35 | 331. | 8.89 | -7.24 | 37.8 | 37.5 |
| Light-Toned Stratified Materials in Melas Chasma: ESP_032747_1690 ESP_033169_1690 (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 | -10.5 | 285. | -2.6 | -24.4 | 35.6 | 42.1 |
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