Influence of the solar-wind magnetic field on the magnetosheath turbulence behind the bow shock
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- Type
- article
- Published
- 2001-12-01
- Cited by
- 5
- References
- 6
- OpenAlex
- https://openalex.org/W41464315
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:116397334
Keywords
Physics, Magnetosheath, Solar wind, Bow shock (aerodynamics), Magnetosphere
References
- Neural computing: theory and practice
- AMPTE observations of mirror mode waves in the magnetosheath: Wavevector determination
- Simulation of pressure pulses in the bow shock and magnetosheath driven by variations in interplanetary magnetic field direction
- Electrodynamics of continuous media (in Russian)
- Electrodynamics of continuous media
- The theory of homogeneous turbulence
- The Theory of Homogeneous Turbulence
- Electrodynamics of Continuous Media
Cited by
- Geomagnetic substorm activity associated with magnetic clouds
- Small-Scale Turbulence of the Earth’s Magnetosheath
- The “Sura” facility: Study of the atmosphere and space (a review)
- Dependence of the Geomagnetic Activity on the Structure of Magnetic Clouds
- Substorm Activity and Orientation of the Front of a Shock Wave of an Interplanetary Magnetic Cloud
- MHD waves at the pre-front of interplanetary shocks on September 6 and 7, 2017
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