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.
Lava Flow Margin in Amazonis Planitia: PSP_008804_2055 PSP_009226_2055 (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 | 25.51 | 192. | 6.80 | -18.1 | 43.1 | 46.4 |
Small Shield in Syria Planum: PSP_008894_1685 PSP_009962_1685 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.2 | 260. | -11. | 6.842 | 62.0 | 61.2 |
Tightly-Meandering Ridge in Aeolis Planum: PSP_008621_1750 ESP_016269_1750 (Interval in Earth days: 596) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.93 | 154. | -8.3 | -26.0 | 56.9 | 48.9 |
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 |
Light-Toned Outcrops in Noctis Labyrinthus: PSP_009118_1665 ESP_028080_1665 (Interval in Earth days: 1478) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.4 | 263. | 5.47 | -16.3 | 62.9 | 60.4 |
Light Toned Materials and Plains in South Meridiani (MSL): PSP_009497_1770 PSP_009919_1770 (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 | -3.03 | 354. | 5.85 | -8.49 | 56.9 | 57.9 |
Layered Rocks in Northern Hellas Planitia: PSP_008756_1510 PSP_008967_1510 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.8 | 69.8 | 7.46 | -14.8 | 72.4 | 74.3 |
Central Peak of Well-Preserved Crater Northwest of Tartarus Montes: PSP_009240_2055 ESP_017943_2055 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.01 | 167. | 6.15 | -17.6 | 44.5 | 45.1 |
Tongue-Shaped Feature on Slope Seen in MOC Images R04-02106 and R12-01135: PSP_008519_2210 PSP_009020_2210 (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 | 40.73 | 52.4 | 7.81 | -1.65 | 41.2 | 42.8 |
Outcrop of Light-Toned Deposit South of Coprates Chasma: PSP_009143_1645 ESP_052737_1645 (Interval in Earth days: 3397) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.1 | 301. | -4.2 | 13.31 | 64.6 | 59.4 |
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