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.
| Layered Blocks Leaning against Slopes in Deuteronilus Mensae : ESP_028273_2240 ESP_028418_2240 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.59 | 26.3 | -3.6 | 10.66 | 53.9 | 54.6 |
| 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 |
| West Candor Chasma Layering : ESP_028422_1730 ESP_026378_1730 (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 | -6.73 | 284. | 8.76 | -8.93 | 55.0 | 56.8 |
| 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 |
| 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 |
| Layered Deposits in West Candor Chasma : ESP_028211_1735 ESP_028277_1735 (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 | -6.60 | 284. | 9.17 | -11.9 | 55.3 | 56.8 |
| Secondaries of Very Fresh Crater : ESP_028569_2235 ESP_033817_2235 (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 | 43.37 | 225. | 2.51 | -9.66 | 57.3 | 44.9 |
| 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 |
| 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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