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.
| Interaction of Modified Ejecta with Tectonic Features in Ascuris Planum : ESP_045525_2235 ESP_045248_2235 (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 | 42.98 | 278. | 6.02 | 19.25 | 45.9 | 42.3 |
| Stratified Material in Tithonium Chasma : ESP_045486_1750 ESP_062022_1750 (Interval in Earth days: 1289) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.84 | 270. | 6.77 | 24.95 | 52.1 | 54.3 |
| Dunes Buried by Water Ice : ESP_045592_2625 ESP_045777_2625 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.30 | 223. | 6.95 | -7.67 | 66.6 | 69.9 |
| Exposure of North Polar Layered Deposits : ESP_045625_2615 ESP_045599_2615 (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 | 81.24 | 44.7 | 8.37 | -6.57 | 66.3 | 66.7 |
| Beautiful Blocks of Bedrock: ESP_044902_1575 ESP_044968_1575 (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 | -22.1 | 13.9 | 2.01 | -16.6 | 65.0 | 65.9 |
| Fractured Crater Fill : ESP_045522_2175 ESP_045588_2175 (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 | 36.97 | 1.48 | 8.69 | -9.68 | 44.3 | 46.6 |
| Breached Crater Near Marte Vallis : ESP_045634_2035 ESP_045924_2035 (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 | 23.36 | 185. | 6.26 | 26.04 | 44.5 | 45.0 |
| Lava Channel in Eastern Amazonis Planitia : ESP_045765_1995 ESP_046187_1995 (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 | 19.13 | 210. | -0.0 | -18.6 | 46.2 | 51.0 |
| Floor of Maja Valles : ESP_045564_1860 ESP_046131_1860 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.044 | 299. | 4.54 | -6.00 | 47.7 | 50.0 |
| 65-Meter Diameter Crater on North Residual Ice : ESP_045448_2730 ESP_062893_2730 (Interval in Earth days: 1360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.98 | 98.2 | -1.4 | -10.6 | 71.2 | 70.1 |
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