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.
| Flow Margin in Phlegra Dorsa : ESP_059744_2080 ESP_059599_2080 (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 | 27.55 | 173. | 8.20 | -6.31 | 37.9 | 39.6 |
| Well-Preserved Crater South of Acidalia Planitia : ESP_059579_2225 ESP_077159_2225 (Interval in Earth days: 1370) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.12 | 356. | 1.21 | -18.1 | 47.4 | 52.1 |
| Layers around Mound in Northern Mid-Latitudes : ESP_059709_2250 ESP_069034_2245 (Interval in Earth days: 726) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.83 | 47.5 | -5.3 | 10.52 | 48.2 | 49.6 |
| Craters : ESP_059632_1470 ESP_060199_1470 (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 | -32.5 | -0.9 | 2.00 | 12.09 | 51.1 | 59.5 |
| Noachis Terra Sand Dune Topography : ESP_059619_1400 ESP_059975_1400 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 355. | -2.5 | 8.852 | 56.1 | 61.3 |
| Pitted Cones in Coprates Chasma : ESP_059621_1665 ESP_059977_1665 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 297. | -8.7 | 5.354 | 40.0 | 43.9 |
| Small Gullies and Fans along Ridge in Nereidum Montes : ESP_059647_1360 ESP_059502_1360 (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 | -43.9 | 309. | 20.8 | 8.562 | 58.6 | 56.8 |
| Valleys in Crater North of Sacra Sulci : ESP_059608_2110 ESP_059753_2110 (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 | 30.93 | 287. | -7.6 | 6.675 | 41.2 | 39.4 |
| Crater Floor Deposits : ESP_059538_2065 ESP_060250_2065 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.17 | 38.7 | -7.1 | 17.25 | 39.3 | 36.2 |
| Pitted Mounds in Chryse Planitia : ESP_059646_2245 ESP_059712_2245 (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 | 44.09 | 325. | 8.76 | -5.79 | 47.5 | 47.8 |
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