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.
| Crater Rim Breach: ESP_083932_1715 ESP_084657_1715 (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 | -8.28 | 131. | 0.56 | 21.48 | 43.7 | 34.7 |
| South Polar Carbon Dioxide Glacier Crevasses: ESP_083884_0930 ESP_075221_0930 (Interval in Earth days: 675) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.9 | 20.2 | 24.9 | 12.53 | 63.3 | 64.8 |
| Crater with Hydration Signatures in West Hellas Planitia: ESP_083988_1400 ESP_084568_1400 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.7 | 47.2 | -0.7 | 13.85 | 39.6 | 37.9 |
| Channels in Tyrrhena Terra: ESP_083802_1595 ESP_092913_1595 (Interval in Earth days: 710) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.4 | 83.8 | -6.9 | 13.89 | 41.9 | 36.5 |
| Light-Toned Outcrops in Osuga Valles: ESP_083701_1645 ESP_084136_1645 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.2 | 321. | -8.4 | 3.583 | 44.5 | 38.6 |
| Pit in Residual Ice Cap: ESP_083943_0920 ESP_074975_0920 (Interval in Earth days: 699) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 232. | 19.1 | 29.01 | 64.7 | 63.6 |
| Narrow South Polar Carbon Dioxide Deposit: ESP_083891_0920 ESP_075490_0920 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 211. | 19.1 | 29.16 | 64.6 | 66.4 |
| USGS Dune Database Entry Number 1978-657: ESP_083719_1140 ESP_084141_1140 (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 | -65.7 | 197. | 1.21 | -19.9 | 51.5 | 52.4 |
| Light Layers at Base of Mounds in Oxia Colles: ESP_084096_2010 ESP_084320_2010 (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 | 20.63 | 330. | -8.3 | 22.19 | 59.3 | 54.8 |
| Inverted Channel in Arabia Terra: ESP_083792_1895 ESP_083726_1895 (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 | 9.630 | 354. | -24. | 1.823 | 56.6 | 55.5 |
Page 71 of 891 (8,901 images) | |||||