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.
| Channels near Huygens Crater: ESP_076880_1615 ESP_077091_1615 (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 | -18.2 | 56.4 | -6.7 | 14.11 | 41.6 | 42.9 |
| Ripple Change Detection of Gullied Dunes in Southern Mid-Latitudes: ESP_076842_1275 ESP_076710_1275 (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 | -51.9 | 18.1 | -1.8 | 18.56 | 60.6 | 57.2 |
| Layered Deposits in Impact Crater in Utopia Planitia: ESP_076984_2240 ESP_077960_2240 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.81 | 89.5 | -1.1 | -11.8 | 53.7 | 46.9 |
| Monitoring the Slopes of Moni Crater: ESP_077053_1325 ESP_085268_1325 (Interval in Earth days: 640) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.0 | 18.7 | -0.8 | -16.4 | 60.7 | 51.5 |
| Streamlined Landforms Adjacent to Shalbatana Vallis: ESP_076989_1895 ESP_076923_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 | 9.220 | 317. | -0.6 | 13.62 | 38.2 | 37.0 |
| 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 |
| Small Delta or Fan: ESP_076729_1755 ESP_075964_1755 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.60 | 217. | -24. | -6.35 | 38.5 | 37.1 |
| 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 |
Page 117 of 878 (8,771 images) | |||||