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.
| Wallrock Spurs That Are Alligned and Extend Into Melas Chasma: ESP_016528_1705 ESP_016884_1705 (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 | -9.28 | 282. | -8.6 | 5.446 | 52.4 | 54.7 |
| Very Large Pit Crater in Daedalia Planum: ESP_016411_1605 ESP_024481_1605 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.4 | 237. | 0 | -21.9 | 56.8 | 47.0 |
| Columnar Jointing in West Wall of Crater in Marte Vallis: ESP_016360_2020 ESP_016505_2020 (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 | 21.55 | 184. | 7.23 | 21.49 | 39.4 | 38.5 |
| Discontinuous Small Channel South of Dao Vallis: ESP_016311_1420 ESP_016588_1420 (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 | -37.6 | 89.5 | 5.56 | -17.0 | 67.7 | 72.4 |
| Isolated Layered Mound in Trough Between Layered Benches in Terby Crater: ESP_016628_1520 ESP_016773_1520 (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 | -27.6 | 74.4 | 0.18 | 16.62 | 64.9 | 65.4 |
| Central Uplift and Olivine-Rich Ponded Material in Elorza Crater: ESP_016659_1710 ESP_017081_1710 (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 | -8.77 | 304. | 10.5 | -3.93 | 52.2 | 56.4 |
| Crater in Acidalia Planitia: ESP_016841_2340 ESP_017830_2340 (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 | 53.72 | 7.48 | 5.69 | -6.67 | 45.4 | 44.9 |
| Debris Apron Source Area: ESP_016673_2255 ESP_017741_2255 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.29 | 276. | -1.2 | 10.92 | 43.4 | 41.3 |
| 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 |
| 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 |
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