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.
| South Polar Residual Cap in Late Summer: ESP_032565_0910 ESP_032538_0910 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.9 | 280. | 23.2 | 25.63 | 84.9 | 84.2 |
| Migrating and Static Sand Ripples on Mars: ESP_032616_1275 ESP_032748_1275 (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 | -52.2 | 267. | 3.02 | -26.0 | 56.8 | 60.7 |
| Lava against an Impact Crater in Elysium Planitia: ESP_018537_1860 ESP_019170_1860 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.980 | 150. | 5.55 | -19.2 | 51.1 | 53.8 |
| Possible Cyclic Bedding within a Crater in Arabia Terra: ESP_018714_1890 ESP_019347_1890 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.969 | 358. | 6.46 | -18.9 | 50.0 | 53.4 |
| Pitted Terrain Associated with Lava Flow: ESP_032395_2070 ESP_032672_2070 (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 | 26.74 | 170. | -0.5 | -26.7 | 46.1 | 45.3 |
| Exposure of South Polar Layered Deposits: ESP_032401_0920 ESP_032650_0920 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.9 | 93.8 | 8.93 | 20.48 | 82.8 | 85.6 |
| Margin of Pedestal Crater in Malea Planum: ESP_032440_1225 ESP_032572_1225 (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 | -56.9 | 32.9 | 5.48 | -22.0 | 57.2 | 61.0 |
| Lava Flow in Syria Planum: ESP_032326_1605 ESP_032827_1605 (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 | -19.1 | 259. | 7.00 | 25.67 | 33.4 | 37.6 |
| South Polar Residual Cap in Summer: ESP_032390_0925 ESP_032521_0925 (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 | -87.3 | 5.67 | 8.59 | 19.38 | 81.5 | 82.7 |
| Dark V-Shaped Feature Cutting across Layers or Bands on a Slope: ESP_032227_2040 ESP_040271_2040 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.62 | 78.8 | -8.7 | 3.583 | 46.4 | 56.7 |
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