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.
| Pitted Cones in Aurorae Chaos: ESP_088540_1720 ESP_089107_1720 (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 | -7.77 | 320. | 3.86 | -8.75 | 60.1 | 60.9 |
| Layering and Contact in Lucus Planum: ESP_088545_1725 ESP_088756_1725 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.43 | 184. | -3.0 | -16.9 | 60.3 | 61.4 |
| Jezero Crater: ESP_088707_1985 ESP_088773_1985 (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 | 18.47 | 77.5 | 0.57 | -21.6 | 47.7 | 49.7 |
| Stunning Outcrop in Nilosyrtis Mensae: ESP_088681_2160 ESP_088892_2160 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.47 | 65.6 | -5.2 | -14.7 | 44.7 | 46.4 |
| Monitoring Gullied Crater: ESP_088568_2310 ESP_088634_2310 (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 | 50.71 | 266. | 8.41 | -6.17 | 44.4 | 45.9 |
| Lobate Glacial Deposit in Crater: ESP_088601_2150 ESP_088825_2150 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.85 | 90.4 | -8.8 | 26.07 | 44.8 | 42.4 |
| North Polar Residual Cap Topography: ESP_088751_2685 ESP_089016_2685 (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 | 88.39 | 276. | -17. | -26.2 | 64.2 | 66.2 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088500_2435 ESP_088421_2435 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 62.98 | 320. | 7.80 | -6.45 | 48.1 | 49.1 |
| Crater and Flow in Daedalia Planum: ESP_088557_1685 ESP_089058_1685 (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 | -11.5 | 217. | -8.9 | 3.217 | 63.3 | 62.3 |
| Wrinkle Ridge and Valley Network Intersection: ESP_088616_1750 ESP_088471_1750 (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 | -4.96 | 45.5 | -4.8 | -15.5 | 59.1 | 59.6 |
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