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.
| Sinuous Ridge with Mesa at Terminus in Kasabi Crater: ESP_034508_1520 ESP_035154_1520 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.7 | 89.1 | -6.1 | 19.81 | 67.4 | 70.3 |
| Channels on Mesa in Southern Elysium Planitia: ESP_034558_1775 ESP_052307_1775 (Interval in Earth days: 1383) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.48 | 159. | 6.18 | 26.96 | 50.8 | 47.7 |
| Spectacular Bedrock Exposures in Walls of Coprates Chasma: ESP_034777_1650 ESP_017503_1650 (Interval in Earth days: 1346) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.0 | 303. | -14. | 3.076 | 61.4 | 62.3 |
| Lava Textures inside Kasei Valles: ESP_034724_2065 ESP_035568_2065 (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 | 26.17 | 303. | 4.53 | -23.0 | 41.0 | 45.8 |
| Low Albedo Slopes along Coprates Chasma Ridge: ESP_034619_1670 ESP_034830_1670 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.9 | 295. | 6.13 | -6.21 | 57.6 | 59.8 |
| Small Crater with Faded Rays: ESP_034854_1870 ESP_036911_1870 (Interval in Earth days: 160) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.076 | 357. | 1.36 | 24.51 | 48.1 | 51.3 |
| Ring Depressions in Scalloped Terrain: ESP_034653_2250 ESP_034165_2250 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.57 | 82.3 | -18. | 9.678 | 43.7 | 42.4 |
| Fractured Surface in Avernus Region: ESP_034505_1770 ESP_034795_1770 (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 | -2.74 | 167. | -3.6 | 20.02 | 51.2 | 51.6 |
| Marte Vallis Lava: ESP_034544_1885 ESP_034834_1885 (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 | 8.43 | 180. | 5.50 | 27.28 | 45.4 | 45.2 |
| A Landing Site in Ladon Vallis: ESP_034987_1595 ESP_035053_1595 (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 | -20.2 | 329. | -3.0 | -24.8 | 65.5 | 67.2 |
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