Nonlinear Alfven waves in high-speed solar wind streams
Journal Article
·
· J. Geophys. Res.; (United States)
A nonlinear proton distribution function that is an exact stationary solution of the nonlinear Vlasov equation and Maxwell's equations and which supports a single nonlinear transverse Alfven (ion cyclotron) wave that is circularly polarized and nondisprsive is proposed for most of the observations during high-speed solar wind streams. This nonlinear distribution removes the strong Alfven wave instability, inconsistent with the persistence of the observed proton distribution functions in high-speed streams, found by the linear stability analysis. Model temperature anisotropies and drift velocities of the two spatially inhomogeneous bi-Maxwellian components are consistent with typical proton velocity distributions measured in high-speed streams at 1 AU. Two derived relations for each of the wave number and the phase velocity of the wave are obeyed within experimental uncertainties by two typical proton measurements. Our model also predicts that the alpha particle bulk flow velocity exceeds the proton particle bulk flow velocity, as is observed.
- Research Organization:
- University of California, Los Alamos Scientific Laboratory, Los Alamos, New Mexico 87545
- OSTI ID:
- 7312374
- Journal Information:
- J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 82:4; ISSN JGREA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Nonlinear alfven waves in high speed solar wind streams
Proton-driven electromagnetic instabilities in high-speed solar wind streams
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Journal Article
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Mon Jan 31 23:00:00 EST 1977
· J. Geophys. Res.; (United States)
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OSTI ID:5085901
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Journal Article
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Wed Jan 31 23:00:00 EST 1979
· J. Geophys. Res.; (United States)
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OSTI ID:6326240
A KINETIC ALFVEN WAVE AND THE PROTON DISTRIBUTION FUNCTION IN THE FAST SOLAR WIND
Journal Article
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Fri Aug 20 00:00:00 EDT 2010
· Astrophysical Journal Letters
·
OSTI ID:21450950
Related Subjects
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ALFVEN WAVES
BARYONS
BOLTZMANN-VLASOV EQUATION
COSMIC PROTONS
COSMIC RADIATION
DIFFERENTIAL EQUATIONS
DISTRIBUTION FUNCTIONS
ELEMENTARY PARTICLES
EQUATIONS
FERMIONS
HADRONS
HYDROMAGNETIC WAVES
INSTABILITY
IONIZING RADIATIONS
NUCLEONS
PLASMA INSTABILITY
PROTONS
RADIATIONS
SOLAR ACTIVITY
SOLAR WIND
TEMPERATURE DISTRIBUTION
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ALFVEN WAVES
BARYONS
BOLTZMANN-VLASOV EQUATION
COSMIC PROTONS
COSMIC RADIATION
DIFFERENTIAL EQUATIONS
DISTRIBUTION FUNCTIONS
ELEMENTARY PARTICLES
EQUATIONS
FERMIONS
HADRONS
HYDROMAGNETIC WAVES
INSTABILITY
IONIZING RADIATIONS
NUCLEONS
PLASMA INSTABILITY
PROTONS
RADIATIONS
SOLAR ACTIVITY
SOLAR WIND
TEMPERATURE DISTRIBUTION