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.
| 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 |
| Valley in Crater : ESP_043341_1685 ESP_044119_1685 (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 | -11.3 | 146. | -1.8 | 7.619 | 55.2 | 58.0 |
| Proposed Site for Future Exploration on Western Side of Ladon Valles : ESP_043242_1600 ESP_044719_1600 (Interval in Earth days: 116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.9 | 329. | 2.38 | -8.20 | 59.8 | 64.6 |
| 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 |
| Pit in Eastern Noctis Labyrinthus with Jarosite : ESP_043363_1725 ESP_043719_1725 (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 | -7.65 | 267. | -24. | -11.6 | 54.6 | 55.6 |
| 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 |
| Dark Dunes Superimposed on Light Bedforms in MOC E01-01076 : ESP_043442_1730 ESP_044009_1730 (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 | -6.73 | 267. | 5.82 | 18.1 | 52.5 | 54.1 |
| Possible Crustal Carbonate Remnant Butte : ESP_043322_2295 ESP_043599_2295 (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 | 49.16 | 296. | 0.31 | -15.7 | 42.9 | 43.3 |
| Layered Bedrock in Terby Crater : ESP_043225_1525 ESP_043937_1525 (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 | -27.3 | 75.1 | -0.4 | 23.99 | 65.1 | 68.0 |
| Braided Channel in the Southern Highlands : ESP_043261_1440 ESP_045226_1440 (Interval in Earth days: 153) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.7 | 174. | -6.7 | -21.5 | 71.8 | 74.2 |
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