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Magnetic storm
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High Quality Content by WIKIPEDIA articles! A geomagnetic storm is a temporary disturbance of the Earth's magnetosphere caused by a disturbance in space weather. Associated with solar coronal mass ejections (CME), coronal holes, or solar flares, a geomagnetic storm is caused by a solar wind shock wave which typically strikes the Earth's magnetic field 24 to 36 hours after the event. This only happens if the shock wave travels in a direction toward Earth. The solar wind pressure on the magnetosphere will increase or decrease depending on the Sun's activity. These solar wind pressure changes modify the electric currents in the ionosphere. Magnetic storms usually last 24 to 48 hours, but some may last for many days. In 1989, an electromagnetic storm disrupted power throughout most of Quebec and caused auroras as far south as Texas. From August 28 until September 2, 1859, numerous sunspots and solar flares were observed on the sun, the largest flare occurring on September 1.
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786131667367
- Genre Geowissenschaften
- Editor Frederic P. Miller, Agnes F. Vandome, John McBrewster
- Anzahl Seiten 68
- Herausgeber Alphascript Publishing
- EAN 9786131667367
- Format Kartonierter Einband
- Titel Magnetic storm
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