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.
Ridges and Mounds Near Hecates Tholus: PSP_007672_2155 PSP_007883_2155 (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 | 34.92 | 142. | 6.64 | -7.98 | 40.8 | 42.0 |
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 |
Large Dunes Possibly of Aqueous Origin in Gale Crater: PSP_007356_1750 PSP_008147_1750 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.19 | 137. | -4.1 | 6.367 | 46.5 | 53.3 |
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 |
Blocky Deposit and Valley Networks Along Melas Chasma Wallrock: PSP_007443_1705 PSP_007733_1705 (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 | -9.17 | 282. | -9.1 | 5.346 | 49.8 | 52.0 |
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 |
Fading Rayed Crater in Daedalum Planum: PSP_007735_1570 ESP_028345_1570 (Interval in Earth days: 1606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 230. | 2.03 | -10.9 | 60.9 | 63.5 |
Unnamed Well-Preserved Crater in Terra Cimmeria: PSP_007000_1475 PSP_007145_1475 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.0 | 141. | -1.0 | 10.11 | 57.0 | 58.6 |
Libya Montes Hydrated Minerals: PSP_007503_1840 ESP_024526_1840 (Interval in Earth days: 1326) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.763 | 82.2 | -3.4 | 22.04 | 44.2 | 35.1 |
Circular Feature with Layers of Repeated Thickness and Expression: PSP_007427_1820 PSP_007862_1820 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.331 | 357. | -0.1 | 20.72 | 44.2 | 46.5 |
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