Lunar magnetic anomalies are locally strong magnetic fields near the Moon caused by permanently magnetized material in its upper crust. They have scale sizes of up to hundreds of kilometers and were first detected by magnetometers on the Apollo 15 and 16 subsatellites in 1971 and 1972 (Coleman et al. 1972). Some of these anomalies probably have surface fields as strong as several thousand nanoTeslas (nT) but fields at orbital altitudes are typically no more than 5 or 10 nT. Major applications of lunar magnetic anomalies include investigating: (a) the existence and history of a former lunar core dynamo; (b) the magnetic effects of large-scale impacts on the Moon; and (c) the role of the solar wind ion bombardment in producing space weathering or optical maturation (darkening with time) of airless silicate bodies in the solar system. Most recently, lunar magnetic anomalies have been mapped using magnetometer data from the Lunar Prospector and Kaguya (SELENE) orbital missions in...
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Hood, L.L. (2014). Lunar Magnetic Anomalies. In: Cudnik, B. (eds) Encyclopedia of Lunar Science. Springer, Cham. https://doi.org/10.1007/978-3-319-05546-6_4-1
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