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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Ground-based diagnostics of the electromagnetic environment of solar activity and natural disasters

Boytchev, B.V.; Nenovski, P.I. Recent Advances in Space Technologies, 2003. RAST '03. International Conference on. Proceedings of, 2003

On the base of theoretical considerations concerning the nature of ultra-low frequency (ULF) signals (both of magnetospheric and lithospheric origin) an instrument for ULF electric and magnetic field measurements is designed and put in operation on the ground. By this apparatus a continuous monitoring of the ULF electromagnetic environment is realised.


Modes in rectangular guides partially filled with transversely magnetized ferrite

Barzilai, G.; Gerosa, G. Antennas and Propagation, IRE Transactions on, 1959

A general modal solution for a rectangular guide partially filled with a slab of ferrite transversely magnetized and situated against one side wall is considered. The relative characteristic equation, which has been obtained in a previous work, is numerically solved for some typical cases and for modes of zero, first and second order with respect to the dependence along the ...


Integrated Multispeed Magnetic Gears: A Novel Approach to Design of Magnetic Transmission Systems

Rashidi, H.; Pishdad, D. Magnetics, IEEE Transactions on, 2015

In this paper, a novel approach for the design of magnetic gears is proposed to provide various gear ratios per unit in a magnetic gear system, including a stator, a rotor, and steel segments. This design utilizes rod-shaped permanent magnets in the stator complex instead of arc-shaped permanent magnets used in ordinary magnetic gear systems. Interestingly, the number of pole ...


Concept for a new frontiers mission to Ganymede: A Planetary Science Summer School study

Jones, B.; Vogt, M.F.; Chaffin, M.; Choukroun, M.; Ehsan, N.; Gibbons, L.; Lynch, K.; Singer, K.; Blackburn, D.; DiBraccio, G.; Gleeson, D.; Le Gall, A.; McEnulty, T.; Rampe, E.; Schrader, C.; Seward, L.; Smith, I.; Tsang, C.; Williamson, P.; Castillo, J.; Budney, C. Aerospace Conference, 2011 IEEE, 2011

As part of the NASA Planetary Science Summer School 2010, the Ganymede Interior, Surface and Magnetosphere Observer (GISMO) team developed a robotic mission to Ganymede, one of Jupiter's icy moons. This process included the formulation of the science objectives and the selection of a payload tailored to meet these goals. The team then designed a mission architecture aimed toward achieving ...


Ordering intermetallic alloys by ion irradiation: a new way to tailor magnetic media

Ravelosona, D.; Menendez, J.I.; Attane, J.P.; Bernas, H.; Halley, D.; Heinig, K.-H.; Marty, A.; Auric, P.; Chappert, C.; Samson, Y. Magnetics Conference, 2003. INTERMAG 2003. IEEE International, 2003

In this paper, we describe ordering mechanism under irradiation by combining experiments and Kinetic Lattice Monte Carlo (KLMC) simulations on the FePt and FePd equiatomic systems. Both experiments and simulations confirm that our irradiation conditions (small energy transfer, low collision cross section, irradiation temperature under 550K) specifically affect DSRO.


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