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.
| North-Pole-Facing Deposit in Crater: ESP_086670_2255 ESP_087593_2255 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.94 | 248. | -4.3 | 8.242 | 46.9 | 42.7 |
| Possible Thin Glacial Lobe in Young Crater: ESP_086309_1490 ESP_086810_1490 (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 | -30.4 | 35.6 | -7.9 | 3.638 | 56.9 | 63.4 |
| Fluvial Valley South of Ares Vallis: ESP_086311_1890 ESP_087168_1890 (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 | 9.094 | 335. | 4.24 | 24.34 | 39.5 | 43.5 |
| Thermophysical Boundary West of Hebrus Valles: ESP_086345_2015 ESP_087123_2015 (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 | 21.09 | 124. | 5.18 | -9.06 | 39.9 | 43.0 |
| Features around Cerberus Palus: ESP_086252_1850 ESP_086819_1850 (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 | 4.904 | 146. | 5.75 | -7.57 | 39.5 | 45.0 |
| Crater in Cerberus Fossae: ESP_086212_1890 ESP_086858_1890 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.700 | 158. | 4.61 | 25.42 | 38.9 | 41.3 |
| Lethe Vallis Chevron Shaped Landforms: ESP_086344_1840 ESP_086845_1840 (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 | 4.028 | 155. | -7.9 | 5.786 | 41.4 | 44.5 |
| 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 |
| 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 |
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