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.
| Intracrater Dune Field Changes: ESP_086695_1360 ESP_086761_1360 (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 | -43.7 | 297. | -0.1 | -18.3 | 71.4 | 73.4 |
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_086671_2205 ESP_087093_2205 (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 | 40.33 | 220. | 6.96 | -3.98 | 44.2 | 43.7 |
| North Mid-Latitude Dune Field Topography: ESP_086760_2420 ESP_087195_2420 (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 | 61.54 | 308. | -2.2 | 17.53 | 54.7 | 49.8 |
| North Pole Facing Deposit in Crater: ESP_086235_2230 ESP_085958_2230 (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 | 42.73 | 248. | -17. | 14.10 | 49.9 | 50.2 |
| Head of Lethe Vallis: ESP_086199_1840 ESP_087056_1840 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.785 | 153. | 5.44 | 20.19 | 39.3 | 45.1 |
| Fluvial Features in Noachis Terra: ESP_086350_1580 ESP_086772_1580 (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 | -21.5 | 353. | 6.39 | -17.1 | 51.1 | 58.3 |
| Hillslope Morphologies Southeast of Ostrov Crater: ESP_086219_1520 ESP_085375_1520 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 332. | -6.1 | 8.78 | 53.6 | 40.3 |
| Gully and Lobate Glacier Fill of Fresh Looking Crater: ESP_086259_2175 ESP_086826_2175 (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 | 37.33 | 311. | 2.92 | -6.63 | 45.5 | 43.8 |
| Mesa Stratigraphy at Terby Crater: ESP_086268_1525 ESP_086835_1525 (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 | -27.1 | 73.7 | 3.54 | -8.39 | 53.5 | 62.3 |
| Margin of Smooth Lobate Deposit in Nereidum Montes: ESP_086259_1405 ESP_085824_1405 (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 | -39.1 | 321. | -1.8 | -16.3 | 61.6 | 55.3 |
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