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.
| Distal Rampart of Toconao Crater: ESP_043125_1590 ESP_043837_1590 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.9 | 284. | -5.6 | 19.06 | 60.0 | 63.2 |
| Clusters of Small Mesas in Northern Arabia Terra : ESP_043201_2160 ESP_043834_2160 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.65 | 1.82 | 5.82 | -4.54 | 39.4 | 39.8 |
| Crater with Intersecting Faults in Tempe Terra : ESP_043283_2220 ESP_043560_2220 (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 | 41.94 | 282. | -0.8 | -19.2 | 40.9 | 41.9 |
| Daedalia Planum Lava Flows : ESP_043219_1570 ESP_045263_1570 (Interval in Earth days: 159) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.8 | 238. | -7.5 | 15.85 | 62.2 | 63.0 |
| Hills in Coprates Chasma : ESP_043177_1655 ESP_042887_1655 (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 | -14.1 | 301. | 23.0 | -6.26 | 54.1 | 53.4 |
| Cratered Lineated Valley Fill : ESP_043159_2145 ESP_043792_2145 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.31 | 68.2 | 9.06 | -2.36 | 39.0 | 39.6 |
| Fans Layers Channels on Floor of Roddy Crater : ESP_043216_1575 ESP_044350_1575 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.0 | 320. | -6.6 | 18.53 | 61.6 | 65.0 |
| Small Fan in Crater West of Mangala Valles : ESP_043418_1640 ESP_043563_1640 (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 | -15.6 | 204. | -3.2 | 14.43 | 58.6 | 58.5 |
| Wrinkle Ridge Near Ganges Catena : ESP_043217_1770 ESP_042716_1770 (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 | -3.08 | 290. | 2.42 | -19.3 | 49.2 | 46.8 |
| Terraced and Rounded Crater Rim in West Utopia Planitia: ESP_043119_2185 ESP_043409_2185 (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 | 38.38 | 81.7 | -9.4 | 14.08 | 41.3 | 38.7 |
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