Publication | Open Access
Importance of post-shock streams and sheath region as drivers of intense magnetospheric storms and high-latitude activity
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Citations
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References
2004
Year
Solar Wind CausesEngineeringSolar ConvectionSolar-terrestrial InteractionSolar PhysicEarth ScienceGeophysicsSolar Terrestrial EnvironmentAtmospheric ScienceMagnetohydrodynamicsSpace PhysicSolar WindPlanetary MagnetosphereSolar ActivitySolar Wind DriverHigh-latitude ActivitySpace Weather EventsMagnetic DisturbancesSpace WeatherMagnetospheric PlasmaSolar VariabilityPost-shock StreamsIonosphereMagnetospheric PhysicsSheath Region
Abstract. Magnetic disturbances in the Earth's magnetosphere can be very different depending on the type of solar wind driver. We have determined the solar wind causes for intense magnetic storms (Dst
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