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.
| Layering in North Polar Layered Deposits Trough: PSP_009273_2610 PSP_009365_2610 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.77 | 330. | -4.7 | 8.503 | 58.1 | 57.7 |
| Light-Toned Layering in Plains South of Melas Chasma: PSP_009170_1695 PSP_009803_1695 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.2 | 283. | 8.03 | -15.9 | 60.8 | 62.3 |
| Cerberus Fossae: PSP_008752_1865 PSP_009108_1865 (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 | 6.222 | 174. | 8.31 | -1.93 | 50.1 | 51.9 |
| Anatomy of a Well-Defined Crater Ray Emanating from Gratteri Crater: PSP_008514_1630 ESP_025445_1630 (Interval in Earth days: 1320) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.8 | 197. | -1.3 | -14.6 | 63.5 | 57.2 |
| Platy-Ridged Lavas in Olympus Mons Aureole: PSP_009225_1975 ESP_016227_1975 (Interval in Earth days: 545) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.42 | 218. | 7.78 | -18.4 | 46.6 | 41.4 |
| Zunil Crater Ray Formed within a Dusty Region: PSP_008225_1830 ESP_018510_1830 (Interval in Earth days: 801) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.916 | 167. | -2.7 | 16.38 | 50.1 | 51.7 |
| Characterize Surface Hazards and Science of MSL Rover Landing Site: PSP_008218_1815 PSP_008719_1815 (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 | 1.522 | 357. | 13.4 | -4.22 | 49.6 | 53.4 |
| Stratigraphy in Aureum Chaos: PSP_008443_1760 PSP_008944_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 | -3.72 | 334. | 9.28 | -8.46 | 54.2 | 57.4 |
| Layered Deposit on Crater Floor in Elysium Region: PSP_008305_1890 PSP_008806_1890 (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 | 8.871 | 141. | 6.19 | -11.6 | 47.0 | 50.5 |
| Central Peak and Floor of Large Crater West of Schiaparelli Crater: PSP_008613_1760 PSP_008969_1760 (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 | -3.93 | 12.2 | 1.91 | -18.6 | 55.6 | 58.3 |
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