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.
| Topographically-Deflected Ejecta in Chryse Planitia: PSP_007916_2010 ESP_016078_2010 (Interval in Earth days: 636) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.91 | 322. | 0.50 | 15.41 | 41.8 | 38.0 |
| Craters on an Ice-Rich Debris Apron: PSP_007832_1385 ESP_060736_1385 (Interval in Earth days: 4123) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.3 | 103. | 1.98 | -19.2 | 74.9 | 74.8 |
| Bright Layers in Columbus Crater: PSP_007710_1500 PSP_008066_1500 (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 | -29.6 | 193. | 6.36 | -4.46 | 64.8 | 69.2 |
| Putative Salt Deposits Detected by THEMIS West of Meridiani Region: PSP_007770_1770 PSP_008917_1770 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.17 | 351. | 6.87 | -11.5 | 49.0 | 57.2 |
| Interesting Periglacial Assemblage in Utopia Planitia: PSP_007384_2225 PSP_009467_2225 (Interval in Earth days: 163) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.22 | 86.3 | -1.0 | 14.43 | 44.2 | 43.1 |
| Geometry of Ramparts for Crater in High Southern Latitudes: PSP_007800_1365 PSP_009593_1365 (Interval in Earth days: 139) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.3 | 258. | -5.1 | 7.815 | 76.5 | 83.0 |
| Russell Crater Dunes: PSP_007018_1255 PSP_007229_1255 (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 | -54.2 | 12.9 | 3.27 | -5.25 | 73.2 | 77.0 |
| Santa Fe Crater in Chryse Planitia: PSP_007244_1995 ESP_016052_1995 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.19 | 311. | 5.51 | 19.74 | 38.9 | 37.5 |
| Eroded High-Latitude Mantle: PSP_007159_1405 PSP_007515_1405 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 120. | 6.69 | -4.42 | 64.2 | 69.9 |
| Crater Interior with Light-Toned Rock and Curvilinear Ridge Features: PSP_007465_1595 ESP_085755_1595 (Interval in Earth days: 6100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.2 | 42.9 | -4.0 | -22.9 | 56.2 | 44.2 |
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