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.
Geologic Contacts in Mangala Valles: PSP_007617_1750 PSP_007973_1750 (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 | -4.85 | 209. | 5.90 | -6.28 | 48.4 | 52.6 |
Perplexing Landforms on Hellas Basin Floor: PSP_007135_1400 ESP_016088_1400 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 56.8 | -4.2 | 16.93 | 64.5 | 65.2 |
Alluvial Fan Apex in Saheki Crater: PSP_007543_1580 PSP_007899_1580 (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 | -21.7 | 72.5 | 3.97 | -8.11 | 57.6 | 62.4 |
Layering in Eastern Central Peak of Oudemans Crater: PSP_007193_1700 PSP_008195_1700 (Interval in Earth days: 79) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.89 | 268. | 4.49 | -6.29 | 46.3 | 57.2 |
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 |
Crater with Gullies Seen in MOC Image E14-02164: PSP_007250_1415 ESP_015979_1415 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 155. | 5.87 | -13.0 | 64.8 | 64.5 |
Polar Crater with Summer Ice: PSP_008081_2405 PSP_008793_2405 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 60.34 | 129. | 4.55 | -12.0 | 48.2 | 47.8 |
Putative Salt Deposits Detected by THEMIS West of Meridiani Region: PSP_007981_1770 PSP_008851_1770 (Interval in Earth days: 68) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.06 | 350. | -5.6 | 23.21 | 51.6 | 54.5 |
Deposits in Kasei Valles: PSP_007970_2015 ESP_033551_2015 (Interval in Earth days: 1993) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.06 | 287. | -0.6 | 17.86 | 42.0 | 36.8 |
Possible Sulfates in Coprates Chasma: PSP_007205_1660 ESP_024505_1660 (Interval in Earth days: 1348) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 301. | 5.58 | -16.3 | 48.4 | 44.1 |
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