Kursk Magnetic Anomaly

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File:Map of Russia - Black Earth.svg
Oblasts comprising Central Black Earth Region
File:Bangui anomaly.JPG
Magnetic intensity from satellite data. The Kursk anomaly is the high-intensity (red) anomaly in the north while the Bangui anomaly is the one in central Africa.

The Kursk Magnetic Anomaly (Template:Langx) is recognized as the largest magnetic anomaly on Earth.[1] It is a territory rich in iron ores located within the Kursk, Belgorod, and Voronezh oblasts in Russia, and constitutes a significant part of the Central Black Earth Region.

The Kursk Magnetic Anomaly (KMA) was first discovered in 1773 by the Russian astronomer and academic Pyotr Inokhodtsev while preparing the maps of the General Land Survey (Template:Langx) at the behest of the Russian government. It was not investigated again until 1874 when I. N. Smirnov conducted the first geomagnetic survey of European Russia. In 1883, N. D. Pilchikov, an assistant professor at Kharkiv University, conducted a series of 71 observations of the Kursk Magnetic Anomaly. These revealed a much larger extent than previously measured and for the first time attributed the anomaly to the presence of iron ore. In 1884, on the basis of this discovery, Pilchikov was awarded the silver medal of the Russian Geographical Society.

Serious investigation of the economic potential of the anomaly occurred under the leadership of Ivan Gubkin in 1920–1925, originally based upon the possibilities for oil.[2] Rich ores were discovered in the region of the anomaly about 1931. The ores are spread over an area estimated at Template:Convert and are magnetite quartzites disseminated throughout metamorphic rocks and Pre-Cambrian granitoids. Surveyed ore reserves of ferrous quartzite are presently estimated at more than Template:Convert of 32–37% Fe and more than Template:Convert of 52–66% Fe. The open pit method is used to mine this ore at the Stoylenskoye, Lebedinskoye, and Mikhailovskoye deposits. Underground mining methods are used for the Korobkovskoye deposit.

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