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.
Small Shield Covering the Noctis Fossae: PSP_010305_1780 PSP_010661_1780 (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 | -1.91 | 256. | -7.0 | -0.74 | 57.3 | 56.9 |
High-Latitude Exposure of North Polar Layered Deposits: PSP_010080_2680 PSP_010856_2720 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.79 | 209. | -8.2 | -6.88 | 68.7 | 80.5 |
Possible Flute Casts in Ares Vallis: PSP_009722_1960 PSP_009867_1960 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.92 | 329. | 2.51 | 17.22 | 48.9 | 48.1 |
Light-Toned Deposits and Possible Fluvial Channels on Floor of Ius Chasma: PSP_010146_1720 PSP_010568_1720 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.96 | 277. | -4.7 | -18.8 | 59.9 | 60.5 |
Phyllosilicates in Acidalia Region: PSP_009538_2220 PSP_010039_2220 (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 | 41.78 | 309. | 0.48 | 17.37 | 44.8 | 46.8 |
Fresh 8-Kilometer Diameter Impact Crater: PSP_009625_1900 ESP_016060_1900 (Interval in Earth days: 501) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.793 | 98.5 | 4.97 | -22.4 | 50.7 | 41.9 |
Small Crater on the North Polar Deposits: PSP_009404_2635 PSP_010221_2635 (Interval in Earth days: 63) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.46 | 346. | -3.3 | 12.01 | 60.1 | 66.3 |
High-Latitude Exposure of North Polar Layered Deposits: PSP_010069_2680 PSP_010479_2680 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.94 | 145. | -8.3 | -15.7 | 68.7 | 73.9 |
Central Peak of Crater: PSP_009561_2325 PSP_010260_2325 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 52.40 | 39.8 | 0.54 | -21.0 | 46.6 | 54.9 |
Pitted Knob on Ceti Mensa: PSP_010093_1740 PSP_010515_1740 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.70 | 284. | -6.5 | -19.4 | 59.0 | 59.7 |
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