نتایج جستجو برای: ism alfvén waves

تعداد نتایج: 121170  

2017
Daniel J. Gershman Adolfo F-Viñas John C. Dorelli Scott A. Boardsen Levon A. Avanov Paul M. Bellan Steven J. Schwartz Benoit Lavraud Victoria N. Coffey Michael O. Chandler Yoshifumi Saito William R. Paterson Stephen A. Fuselier Robert E. Ergun Robert J. Strangeway Christopher T. Russell Barbara L. Giles Craig J. Pollock Roy B. Torbert James L. Burch

Alfvén waves are fundamental plasma wave modes that permeate the universe. At small kinetic scales, they provide a critical mechanism for the transfer of energy between electromagnetic fields and charged particles. These waves are important not only in planetary magnetospheres, heliospheres and astrophysical systems but also in laboratory plasma experiments and fusion reactors. Through measurem...

2002
T. Zaqarashvili

We suggest a mechanism for enhancing magnetic activity in tidally interacting binaries. We suppose that the deviation of the primary star from spherical symmetry due to the tidal influence of the companion leads to stellar pulsation in its fundamental mode. It is shown that stellar radial pulsation amplifies torsional Alfvén waves in a dipole-like magnetic field, buried in the interior, accordi...

Journal: :Physical review letters 2012
G G Howes D J Drake K D Nielson T A Carter C A Kletzing F Skiff

Turbulence is a ubiquitous phenomenon in space and astrophysical plasmas, driving a cascade of energy from large to small scales and strongly influencing the plasma heating resulting from the dissipation of the turbulence. Modern theories of plasma turbulence are based on the fundamental concept that the turbulent cascade of energy is caused by the nonlinear interaction between counterpropagati...

2009
J. Martin Laming

We revisit in more detail a model for element abundance fractionation in the solar chromosphere, that gives rise to the “FIP Effect” in the solar corona and wind. Elements with first ionization potential below about 10 eV, i.e. those that are predominantly ionized in the chromosphere, are enriched in the corona by a factor 3-4. We model the propagation of Alfvén waves through the chromosphere u...

Journal: :The Review of scientific instruments 2011
D J Drake C A Kletzing F Skiff G G Howes S Vincena

We have designed an electric and magnetic field probe which simultaneously measure both quantities in the directions perpendicular to the background magnetic field for application to Alfvén wave experiments in the Large Plasma Device at UCLA. This new probe allows for the projection of measured wave fields onto generalized Elsässer variables. Experiments were conducted in a singly ionized He pl...

2007
T. V. Zaqarashvili

The weakly non-linear interaction of slow magnetoacoustic and torsional Alfvén waves propagating along an unperturbed poloidal magnetic field in a stellar interior is studied in the high plasma β limit. It is shown that slow magnetoacoustic waves parametrically drive torsional modes with the half frequency and wave number. Therefore global slow magnetoacoustic waves which have a radial velocity...

2003
G. S. Lakhina B. T. Tsurutani

Two magnetic hole events observed by Polar on 20 May 1996 when it was in the polar cap/polar cusp boundary layer are studied. Low-frequency waves, consisting of nonlinear Alfvén waves and large amplitude (±14 nT peakto-peak) obliquely propagating proton cyclotron waves (with frequency f ∼0.6 to 0.7fcp), accompanied by electric bipolar pulses (electron holes) and electron heating have been obser...

1999
Ethan T. Vishniac

We examine the effect of weak, small scale magnetic field structure on the rate of reconnection in a strongly magnetized plasma. This affects the rate of reconnection by reducing the transverse scale for reconnection flows, and by allowing many independent flux reconnection events to occur simultaneously. Allowing only for the first effect and using Goldreich and Sridhar’s model of strong turbu...

2002
S. S. Komissarov

In this paper we show that switch-on and switch-off shocks are allowed by the shock equations of relativistic MHD and have similar properties to their Newtonian counterparts. Just like in Newtonian MHD they are limits of of fast and slow shock solutions and as such they may be classified as evolutionary shocks. The analysis of Punsly's MHD waveguide problem shows that both fast and Alfvén waves...

2008
Yang Zhang W. W. Heidbrink H. Boehmer R. McWilliams Guangye Chen B. N. Breizman

A multiple magnetic mirror array is formed at the Large Plasma Device LAPD W. Gekelman, H. Pfister, Z. Lucky, J. Bamber, D. Leneman, and J. Maggs, Rev. Sci. Instrum. 62, 2875 1991 to study axial periodicity-influenced Alfvén spectra. Shear Alfvén waves SAW are launched by antennas inserted in the LAPD plasma and diagnosed by B-dot probes at many axial locations. Alfvén wave spectral gaps and co...

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