Bangui magnetic anomaly
The Bangui magnetic anomaly is a local variation in the Earth's magnetic field centered at Bangui, the capital of Central African Republic. The anomaly is roughly elliptical, about 700 km × 1,000 km (430 mi × 620 mi), and covers most of the country, making it one of the "largest and most intense crustal magnetic anomalies on the African continent".[1] The anomaly was discovered in the late 1950s, explored in the 1970s, and named in 1982. Its origin remains unclear.
History
In 1962, Raymond Godivier and Lucien Le Donche reported on a magnetic anomaly in Central African Republic, which they identified by analyzing their surface magnetic activity data of 1956. These results were confirmed and elaborated by the high-altitude aeromagnetic surveys carried out by the US Naval Oceanographic Office, as well as by the satellite measurements conducted in 1964 with Cosmos 49 and in the 1970s with the Orbiting Geophysical Observatory at 350–500 kilometres (220–310 mi) altitudes. These data were combined in 1973 yielding a spatial map of magnetic field, which was updated after the launch of Magsat satellite with an accuracy of 15 nT at an altitude of 400 kilometres (250 mi).[2][3]
In 1982, Robert D. Regan and Bruce D. Marsh named the anomaly after the city in the center of the anomaly.[4]
This anomaly is sometimes called the Bangui negative anomaly, owing to its negative peak-to-trough difference, and is compared with the positive anomalies observed at the Benue trough and Congo Basin where Lower Cambrian geological formations are exposed.[5]
Salient features
The Bangui anomaly is bounded to the south by the Walvis Ridge, the north by the Cameroon–St. Helena volcanic line, and to the west by the Mid-Atlantic Ridge.[1] It is shaped approximately as an ellipse 700 km × 1,000 km (430 mi × 620 mi) in size. It has three sections, and the magnetic equator runs through its center. It has a short axis diameter of about 550 kilometres (340 mi), and its amplitude varies between –1000 nT at ground level and –20 nT at satellite altitude, about 400 kilometres (250 mi).[1] Its features include a Bouguer gravity anomaly of −120 mGal, a topographical surface feature shaped as a ring of 810 km (500 mi) diameter, rock features of Late Archean and Proterozoic periods in the central part of the anomaly, granulites, and charnockites rock formations supplemented by granites at the lower crust level, and greenstone belts, and metamorphosed basalts seen as rock exposures.[2] A zone of thinner crust bounds the anomaly to the north and a zone of relatively thicker crust is on the southern edge.[1]
Origin
Two theories have been suggested for the origin of the Bangui anomaly, neither being conclusive. One attributes it to a large igneous intrusion and the other to a meteorite impact. To support the latter theory, an analogy was drawn with a meteorite impact that occurred in Brazil in Bahia state causing formation of micro-diamond rich carbonates.[2]
References
- 1 2 3 4 Antoine, L. A. G.; Reimold, W. U.; Tessema, A. "The Bangui Magnetic Anomaly Revisited" (PDF). Proceedings 62nd Annual Meteoritical Society Meeting (Lunar and Planetary Institute, Houston). Retrieved 11 April 2013.
- 1 2 3 Gubbins, David; Herrero-Bervera, Emilio (2007). Encyclopedia of Geomagnetism and Paleomagnetism. Springer. pp. 39–40. ISBN 978-1-4020-4423-6.
- ↑ Langel, R. A.; Hinze, W. J. (1998). The Magnetic Field of the Earth's Lithosphere: The Satellite Perspective. Cambridge University Press. pp. 11–12. ISBN 978-0-521-47333-0.
- ↑ Lowman, Paul D. (15 August 2002). Exploring Space, Exploring Earth: New Understanding of the Earth from Space Research. Cambridge University Press. pp. 95, 97. ISBN 978-0-521-89062-5. Retrieved 8 April 2013.
- ↑ Geological Investigations in West Africa. Geological Survey Professional Paper 1275. U.S. Government Printing Office. 1982. p. 255.