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Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure
V. A. Parkhomov
, A. V. Suvorova
, V. G. Eselevich
, S. Yu Khomutov
, M. V. Eselevich
, B. Tsegmed
, A. V. Dmitriev
, T. Raita
太空科學與工程學系
研究成果
:
雜誌貢獻
›
期刊論文
›
同行評審
3
引文 斯高帕斯(Scopus)
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Keyphrases
Solar Wind
100%
Magnetospheric
100%
Diamagnetic Structure
100%
Magnetosphere
85%
Proton
28%
Magnetopause
28%
Radial Direction
14%
Oscillation
14%
Radiation Belts
14%
Bow Shock
14%
Electric Field (E-field)
14%
Postmidnight
14%
Internal Structure
14%
Correlation Coefficient
14%
Geomagnetic Field
14%
Energy Range
14%
Charged Particles
14%
Substorm
14%
Ion Concentration
14%
Earth Orbit
14%
Coronal Mass Ejections
14%
Reconnection
14%
Earth Surface
14%
Aurora
14%
Plasmoid
14%
Near-Earth Orbit
14%
Flow around
14%
Geomagnetic Pulsations
14%
Magnetotail
14%
Classical Model
14%
Sawtooth Substorm
14%
Growth Phase
14%
Ionospheric Currents
14%
Pulsed Electric Field
14%
Auroral Absorption
14%
Earth and Planetary Sciences
Solar Wind
100%
Magnetosphere
100%
International Monetary Fund
33%
Magnetopause
33%
Substorm
33%
Electric Field
33%
Earth Orbit
33%
Geomagnetism
16%
Radiation Belt
16%
Correlation Coefficient
16%
Earth Surface
16%
Flow Structure
16%
Charged Particle
16%
Ionospheric Current
16%
Geomagnetic Pulsation
16%
Plasma Physics
16%
Ion Concentration
16%
Auroral Absorption
16%
Physics
Magnetosphere
100%
Solar Wind
100%
Magnetopause
33%
Stellar Mass Functions
33%
Earth Orbit
33%
Electric Field
33%
Geomagnetism
16%
Ion Concentration
16%
Plasma Physics
16%
Ionospheric Current
16%
Correlation Coefficient
16%
Earth Surface
16%
Geomagnetic Pulsation
16%
Radiation Belt
16%
Charged Particle
16%
Coronal Mass Ejection
16%