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.
| Valleys within Electris Region Deposit: ESP_016664_1420 ESP_045305_1420 (Interval in Earth days: 2232) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.9 | 172. | 1.33 | 28.48 | 72.5 | 72.2 |
| Possible Phyllosilicates: ESP_016891_1710 ESP_017669_1710 (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 | -8.92 | 91.9 | 2.12 | -13.6 | 54.8 | 59.8 |
| Ejecta Flow and Obstacle at Arandas Crater: ESP_016776_2225 ESP_016842_2225 (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 | 42.39 | 344. | 4.98 | -9.79 | 41.8 | 43.0 |
| Small Rampart Crater Near the Central Peak of Lyot Crater: ESP_016326_2305 ESP_060026_2305 (Interval in Earth days: 3405) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.39 | 29.2 | -3.9 | 16.71 | 47.2 | 47.4 |
| Degradation of Old Crater Rim on Northwest Slope of Acheron Fossae: ESP_016873_2185 ESP_017018_2185 (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 | 38.30 | 218. | -8.3 | 1.584 | 42.0 | 41.0 |
| Eroded Material Adjacent to Cerberus Fossae: ESP_016506_1890 ESP_017495_1890 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.114 | 160. | 2.89 | -11.8 | 42.9 | 49.1 |
| Unnamed Crater in Polygonal Terrain in Western Utopia Planitia: ESP_016469_2260 ESP_016535_2260 (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 | 45.59 | 84.3 | 8.50 | -5.58 | 43.4 | 44.2 |
| Terrain South of Newcomb Crater: ESP_016736_1520 ESP_068970_1525 (Interval in Earth days: 4070) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 5.59 | 4.65 | -7.50 | 65.7 | 63.9 |
| Possible Landslide Triggered by Impact: ESP_016386_1475 ESP_016531_1475 (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 | -32.4 | 201. | 1.20 | 16.67 | 65.1 | 65.9 |
| Wrinkle Ridges in Hesperia Planum: ESP_016455_1535 ESP_016811_1535 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.2 | 117. | -5.9 | 7.118 | 62.1 | 65.3 |
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