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.
| Scarp Likely Exposing Polar Layered Deposits in Area Not Well Observed: ESP_013910_0880 ESP_022641_0880 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 216. | 8.73 | 19.64 | 70.6 | 70.3 |
| Central Structure of an Impact Crater: ESP_012636_1490 ESP_013137_1490 (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 | -30.8 | 338. | 6.49 | 28.71 | 47.2 | 38.5 |
| Lineated Valley Fill in Nilosyrtis Mensae: ESP_012883_2135 ESP_013160_2135 (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 | 33.01 | 68.2 | -3.0 | -23.7 | 72.4 | 72.3 |
| Gullied 35 Kilometer Diameter Impact Crater in Promethei Terra: ESP_013660_1475 ESP_013950_1475 (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 | -32.4 | 103. | 0.16 | 23.60 | 36.1 | 33.5 |
| Channel Cutting Wrinkle Ridge in Phlegra Dorsa: ESP_012985_2025 ESP_013130_2025 (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 | 22.00 | 164. | 4.41 | 19.35 | 64.2 | 62.2 |
| Volatiles and Gullies: ESP_013097_1115 ESP_013585_1115 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -68.4 | 1.31 | 2.13 | -13.5 | 53.0 | 53.2 |
| South Polar Layered Deposits Exposed in Ultimum Chasma: ESP_013778_0985 ESP_013659_0985 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.2 | 147. | -12. | 4.816 | 63.8 | 61.6 |
| Warrego Valles Headwater Region: ESP_013153_1390 ESP_013298_1390 (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 | -40.6 | 266. | -5.4 | 6.316 | 42.0 | 39.7 |
| Layered Crater Fill Material: ESP_014017_2085 ESP_022021_2085 (Interval in Earth days: 624) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.99 | 68.5 | 0.69 | 16.01 | 57.5 | 64.7 |
| Eastern Half of Gullied Crater: ESP_012759_1360 ESP_012904_1360 (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 | -43.8 | 222. | 7.98 | 20.17 | 46.7 | 43.7 |
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