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.
| Wind Flow: ESP_057930_1720 ESP_057864_1720 (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 | -8.00 | 25.1 | -1.9 | 12.57 | 34.3 | 34.0 |
| Cross-Section of a Complex Crater : ESP_058057_1465 ESP_058624_1465 (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 | -33.2 | 161. | 5.19 | -17.9 | 31.9 | 37.5 |
| Apollinaris Patera Scarp : ESP_057753_1720 ESP_057542_1720 (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 | -7.94 | 174. | 11.1 | -7.21 | 35.3 | 39.1 |
| Normal Faults along Coprates Chasma Floor : ESP_057854_1670 ESP_057920_1670 (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 | -12.9 | 298. | 8.12 | -6.23 | 32.6 | 33.0 |
| 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 |
| Dipping Layers Near Moreux Crater : ESP_057652_2215 ESP_075614_2215 (Interval in Earth days: 1400) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.40 | 46.2 | -7.8 | 6.251 | 72.3 | 70.0 |
| 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 |
| Dendritic Ridges in Channel Levees : ESP_057649_2055 ESP_066458_2055 (Interval in Earth days: 686) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.02 | 129. | 4.17 | -14.6 | 58.6 | 64.0 |
| 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 |
| Ice Rich Lobate Deposit Flowing from Crater : ESP_057524_1425 ESP_057458_1425 (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 | -37.1 | 309. | -6.9 | 6.893 | 35.4 | 34.9 |
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