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.
| Pavonis Mons Reticulate Bedform Change Detection : ESP_028608_1805 ESP_028542_1805 (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 | 0.517 | 247. | -6.2 | 18.32 | 54.3 | 52.4 |
| Distorted Icy Terrain in Nilosyrtis Mensae Crater : ESP_028601_2145 ESP_028324_2145 (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 | 34.17 | 73.6 | -1.8 | 13.89 | 55.3 | 50.7 |
| Possible Repetitive Bedding Near Base of Central Lobe of Medusae Fossae : ESP_028650_1695 ESP_028795_1695 (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 | -10.4 | 180. | 8.61 | 21.62 | 55.7 | 54.2 |
| Eye of the Beholder: ESP_028957_2085 ESP_046772_2085 (Interval in Earth days: 1388) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.28 | 75.4 | -7.8 | 5.989 | 58.6 | 57.1 |
| What Is It?: ESP_027912_1770 ESP_028611_1770 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.82 | 167. | -7.1 | -25.9 | 55.2 | 56.7 |
| Lobate Flow Features East of Hellas Region: ESP_029035_1455 ESP_029457_1455 (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 | -34.3 | 113. | -7.5 | -21.4 | 62.3 | 58.4 |
| Angular Blocks: ESP_028812_1485 ESP_037396_1485 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.3 | 81.7 | -7.0 | 14.23 | 63.4 | 65.7 |
| The Top of Coprates Chasma: ESP_028962_1645 ESP_037111_1645 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 303. | 5.11 | -21.1 | 56.1 | 62.8 |
| Craters Intersected by Mare-Type Ridges in Lunae Planum : ESP_028580_1900 ESP_029002_1900 (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 | 10.01 | 289. | 11.6 | -6.73 | 51.7 | 55.3 |
| Mid-Latitude Crater with Rayed Ejecta : ESP_028469_2195 ESP_028113_2195 (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 | 39.38 | 75.2 | 8.23 | -8.07 | 54.2 | 51.1 |
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