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.
| Lineations along Medusae Fossae : ESP_028346_1760 ESP_028847_1760 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.17 | 199. | -2.9 | 25.61 | 55.2 | 52.5 |
| Curved and Branching Ridges in CTX B01_009840_1885_XN_08N010W : ESP_028591_1880 ESP_028657_1880 (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 | 7.796 | 349. | 7.78 | -16.1 | 52.2 | 54.5 |
| Complex Superposition of Fractures : ESP_028330_2240 ESP_028620_2240 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.77 | 270. | -9.5 | 17.29 | 55.1 | 57.0 |
| High Thermal Inertia Materials off the Central Peak of Hargraves Crater : ESP_028390_2010 ESP_051097_2010 (Interval in Earth days: 1770) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.72 | 75.7 | -4.6 | -24.7 | 51.5 | 38.2 |
| Western Hellas Planitia : ESP_028589_1380 ESP_037173_1380 (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 | -41.6 | 51.8 | -7.1 | 5.916 | 70.7 | 73.7 |
| Fossae Source of Outflows : ESP_028400_1955 ESP_033371_1955 (Interval in Earth days: 387) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.32 | 163. | -2.4 | 15.52 | 51.5 | 36.0 |
| Cracked Terrain in Argyre Basin : ESP_028500_1425 ESP_028922_1425 (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 | -37.2 | 319. | 6.35 | -7.5 | 68.4 | 64.7 |
| Possible Prehnite and Chlorite Bearing Deposits in Hellas Region : ESP_028536_1535 ESP_028602_1535 (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 | -26.2 | 56.2 | -5.2 | -25.4 | 63.3 | 64.4 |
| Floor of East Candor Chasma : ESP_028514_1720 ESP_028936_1720 (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 | -8.08 | 293. | 8.25 | -9.42 | 55.4 | 55.9 |
| Central Peak of an Impact Crater : ESP_028535_1515 ESP_033783_1515 (Interval in Earth days: 409) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.3 | 83.4 | -0.2 | -16.4 | 64.0 | 59.9 |
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