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Detailed Reference Information |
Kamide, Y. (2006). What is an "Intense Geomagnetic Storm"?. Space Weather 4. doi: 10.1029/2006SW000248. issn: 1542-7390. |
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The main objective of space weather research is to trace the flow of energy from the Sun to the Earth's upper atmosphere. Large changes in the energy input at Earth can seriously affect many technologies. Scientists customarily assume that the best indicator of the intensity of a geomagnetic storm is the minimum value of the Dst index, the longitudinal average of the horizontal component of Earth's low-latitude surface magnetic field. |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Magnetospheric Physics, Magnetic storms and substorms, Magnetospheric Physics, Solar wind/magnetosphere interactions, Ionosphere, Ionospheric storms, Ionosphere, Auroral ionosphere |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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