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.
| Dark Materials on Block in Olympus Mons Aureole: PSP_008935_1975 ESP_016372_1975 (Interval in Earth days: 580) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.33 | 217. | -8.1 | 5.979 | 47.1 | 40.0 |
| 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 |
| 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 |
| 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 |
| Crater Floor and Central Mound in Gale Crater (MSL): PSP_009505_1755 PSP_009571_1755 (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 | -4.47 | 137. | -7.4 | -28.4 | 58.6 | 60.2 |
| Deposits Layered at Several Scales: PSP_009038_1745 PSP_010027_1745 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.54 | 286. | 2.43 | -12.1 | 58.0 | 59.4 |
| Drainage Off Ponded Materials in Mojave Crater: PSP_008496_1880 PSP_009076_1880 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.741 | 326. | -8.6 | 13.58 | 49.6 | 50.0 |
| Polygons and Spots on Defrosting Dunes: PSP_008867_2640 PSP_009105_2640 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.99 | 233. | 8.23 | -9.68 | 59.0 | 59.9 |
| Flows on the Northeastern Flank of Arsia Mons: PSP_008565_1720 PSP_009844_1720 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.68 | 242. | 9.15 | -10.2 | 57.2 | 60.4 |
| Impact Crater Amid the Deuteronilus Mensae: PSP_009021_2245 PSP_009654_2245 (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 | 44.21 | 23.3 | 8.73 | -7.10 | 42.2 | 46.4 |
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