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 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 |
| 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 |
| 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 |
| 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 |
| A Slice through the Layercake: ESP_084979_1975 ESP_085045_1975 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.49 | 336. | 16.6 | -4.34 | 44.6 | 45.3 |
| Transverse Dunes West of Argyre Planitia: ESP_085825_1300 ESP_085759_1300 (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 | -49.8 | 294. | -2.2 | 12.44 | 61.9 | 59.9 |
| Memnonia Sulci: ESP_085921_1735 ESP_086277_1740 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.02 | 186. | 7.83 | -6.28 | 38.7 | 43.5 |
| Hillslope Morphologies in Crater: ESP_085793_1510 ESP_086294_1510 (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 | -28.6 | 84.7 | 3.79 | -4.91 | 47.1 | 55.3 |
| Exposure of Layered Materials along Hellas Planitia Rim Escarpment: ESP_085807_1590 ESP_086242_1590 (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 | -20.7 | 63.1 | -16. | 0.443 | 44.6 | 49.5 |
| Gullied Slope: ESP_085723_1370 ESP_085868_1370 (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 | -42.8 | 197. | -4.7 | 10.24 | 55.4 | 56.9 |
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