Magnetosphere

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A magnetosphere is formed when a stream of charged particles, such as the solar wind, interacts with and is deflected by the intrinsic magnetic field of a planet or similar body. (Wikipedia.org)






Conferences related to Magnetosphere

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2012 International Conference on Electromagnetics in Advanced Applications (ICEAA)

The 14th edition of ICEAA is coupled to the 2nd edition of IEEE-APWC 2012. The two conferences consist of invited and contributed papers, and share a common organization, registration fee, submission site, workshops and short courses, and social events. The proceedings of both conferences will be published on IEEE Xplore.



Periodicals related to Magnetosphere

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Plasma Science, IEEE Transactions on

Plasma science and engineering, including: magnetofluid dynamics and thermionics; plasma dynamics; gaseous electronics and arc technology; controlled thermonuclear fusion; electron, ion, and plasma sources; space plasmas; high-current relativistic electron beams; laser-plasma interactions; diagnostics; plasma chemistry and colloidal and solid-state plasmas.




Xplore Articles related to Magnetosphere

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Using the wavelet transform for the detection of magnetic underwater transient signals

Quinquis, A.; Dugal, C. OCEANS '94. 'Oceans Engineering for Today's Technology and Tomorrow's Preservation.' Proceedings, 1994

In the analysis of transient signals such as those encountered in underwater observations (sonar, magnetic signals) standard Fourier analysis is often not satisfactory. This is because the basis functions of Fourier analysis (sines cosines, complex exponentials) extend over infinite time whereas the signals to be analysed are short-time transients. A new method of dealing with transient signals has recently appeared ...


Hybrid-Vlasov simulations of the Earth's collisionless bow shock and foreshock region

Kempf, Y.; Pokhotelov, D.; von Alfthan, S.; Hannuksela, O.; Palmroth, M. General Assembly and Scientific Symposium (URSI GASS), 2014 XXXIth URSI, 2014

We present magnetospheric simulation results obtained with the hybrid-Vlasov code Vlasiator. In this model, the ion distribution function is propagated in up to three spatial and three velocity dimensions with Vlasov's equation, while electrons are treated as a massless charge-neutralising fluid. Therefore ion kinetic effects are fully included in the description. One major strength of the model is the unprecedented ...


The collinear interaction between forward volume magnetostatic waves and guided light in YIG films

Talisa, Salvador H. Magnetics, IEEE Transactions on, 1988

The TE-to-TM optical mode conversion that takes place when magnetostatic waves (MSW) and a guided light beam propagate collinearly in an yttrium-iron-garnet (YIG) film is investigated. The experimental results show unexpectedly high intensity and broad bandwidth when microwave power levels on the order of 35 dBm are used. This effect is clearly nonlinear, and it is speculated that it could ...


The IMAGE mission and first observations from the radio plasma imager

Reinisch, B.W.; Haines, D.M.; Galkin, I.A.; Green, J.L.; Benson, R.F.; Taylor, W.W.L.; Burch, J.L. Antennas, Propagation and EM Theory, 2000. Proceedings. ISAPE 2000. 5th International Symposium on, 2000

The Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) mission is NASA's first satellite mission designed to image Earth's magnetosphere using remote sensing techniques. Extreme and far ultraviolet (EUV, FUV), energetic neutral atom (ENA), and radio plasma (RPI) imagers are mapping the aurora, the helium ions of the plasmasphere, the plasma sheet and polar cusp, and the total plasma distribution from the ...


Model of diurnal/seasonal variations of ELF natural radio signal based on OTD data

Nickolaenko, A.P. Electromagnetic Compatibility and Electromagnetic Ecology, 2005. IEEE 6th International Symposium on, 2005

Knowledge of expected parameters of natural extremely low frequency (ELF) radio signal arriving from the global lightning activity to observatory is necessary when one looks for the signals originating from other sources, in particular, for the electromagnetic precursors of a future earthquake shock. The radio waves of seismic and cosmic origin might be expected in the bands of ultra-low (ULF, ...


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