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.
| Landslides in Orson Welles Crater: ESP_076910_1805 ESP_085270_1805 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.363 | 314. | 4.79 | 17.67 | 36.9 | 34.8 |
| Volcanic Cone in Claritas Fossae: ESP_076899_1510 ESP_076556_1510 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.5 | 260. | -17. | -2.33 | 47.4 | 41.6 |
| Northwest Argyre Planitia Rim Transverse Dunes: ESP_076871_1355 ESP_076726_1355 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.3 | 304. | 7.15 | -17.7 | 55.3 | 54.3 |
| Terrain Sample: ESP_076970_2000 ESP_077102_2000 (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 | 20.01 | 114. | 7.14 | -18.0 | 40.5 | 42.1 |
| Knobs in East Candor Chasma: ESP_076713_1730 ESP_077201_1730 (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 | -6.83 | 292. | -5.8 | 19.25 | 37.0 | 39.3 |
| Channel-Like Feature: ESP_077076_2250 ESP_077208_2250 (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 | 44.79 | 97.5 | 7.76 | -9.81 | 52.7 | 52.5 |
| Layered Sediments in Southern Arabia Terra: ESP_076750_1835 ESP_076407_1835 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.588 | 1.33 | -2.5 | 17.65 | 37.2 | 35.9 |
| Floor of East Candor Chasma: ESP_077056_1730 ESP_078045_1730 (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 | -6.86 | 291. | -7.9 | 23.88 | 40.0 | 48.6 |
| Lower Interior Layered Deposits in Eastern Candor Chasma: ESP_076845_1730 ESP_076911_1730 (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 | -6.94 | 288. | 8.48 | -6.96 | 36.9 | 38.6 |
| Interaction Between Cone and Ejecta : ESP_076922_2250 ESP_077832_2250 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.42 | 341. | -3.8 | 8.962 | 55.0 | 46.2 |
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