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.
| Dark Dunes and Aeolian Units in Melas Chasma : ESP_057551_1675 ESP_057894_1675 (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 | -12.2 | 289. | -3.5 | -14.3 | 36.9 | 34.1 |
| Ridges and Channels in Light-Toned Unit near Nirgal Vallis: ESP_057537_1540 ESP_057946_1540 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.7 | 312. | 5.46 | -18.2 | 33.4 | 32.3 |
| South Polar Layered Deposits : ESP_057666_0920 ESP_057678_0920 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.7 | 82.2 | 13.8 | 27.19 | 65.8 | 64.8 |
| Crater with Rocky Walls : ESP_057674_1355 ESP_058373_1355 (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 | -44.0 | 176. | -0.4 | -14.4 | 36.4 | 40.6 |
| Valleys in Central Pit Crater Northwest of Hellas Planitia : ESP_057613_1580 ESP_057547_1580 (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 | -21.7 | 38.2 | -4.1 | 11.23 | 33.8 | 33.3 |
| Pit Near Biblis Patera : ESP_057830_1820 ESP_074882_1820 (Interval in Earth days: 1329) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.037 | 232. | -1.0 | 24.46 | 40.5 | 49.5 |
| Slope Features in Arabia Terra : ESP_057878_2115 ESP_058010_2115 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.17 | 356. | 23.5 | 2.71 | 59.8 | 59.1 |
| Erosional Scarp in Mid-Latitude Mantle : ESP_057571_1245 ESP_057782_1245 (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 | -55.1 | 109. | 0.53 | 11.93 | 42.2 | 41.7 |
| Bright Deposits in Channel South of Peraea Cavus : ESP_057545_1495 ESP_057888_1495 (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 | -30.3 | 95.1 | -3.2 | -13.1 | 34.0 | 32.7 |
| Dark Sediments in Medusae Fossae Formation : ESP_057635_1795 ESP_057701_1795 (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 | -0.64 | 154. | 7.71 | -7.69 | 40.7 | 40.9 |
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