Beam-generated plasma turbulence during solar flares

We develop a simple theoretical model to analyze the harmonic plasma radiation produced by an electron beam injected in a flaring loop and traveling along its magnetic field lines. For a given atmospheric model, we consistently consider collisional effects and the generation of Langmuir waves as a f...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	Vasquez, A.M., Gomez, D.O.
Formato:	JOUR
Materias:	Sun: flares Sun: radio radiation Turbulence Waves
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v484_n1PARTI_p463_Vasquez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Beam-generated plasma turbulence during solar flares
Publicado: (1997)

Second harmonic emission during solar flares
por: Vásquez, A.M., et al.

Second harmonic emission during solar flares
Publicado: (2002)

Electrostatic decay of beam-generated plasma turbulence
por: Vásquez, A.M., et al.

Electrostatic decay of beam-generated plasma turbulence
Publicado: (2004)

Rapid submillimeter brightenings associated with a large solar flare
por: Kaufmann, P., et al.

Rapid submillimeter brightenings associated with a large solar flare
Publicado: (2001)

Rapid Submillimeter Brightenings Associated with a Large Solar Flare
por: Kaufmann, Pierre, et al.
Publicado: (2001)

Properties of fast submillimeter time structures during a large solar flare
Publicado: (2003)

Properties of fast submillimeter time structures during a large solar flare
por: Raulin, J.-P., et al.

Magnetohydrodynamic turbulence of coronal active regions and the distribution of nanoflares
por: Dmitruk, P., et al.
Publicado: (1998)

Magnetohydrodynamic turbulence of coronal active regions and the distribution of nanoflares
por: Dmitruk, P., et al.

Magnetohydrodynamic turbulence of coronal active regions and the distribution of nanoflares
por: Dmitruk, P., et al.
Publicado: (1998)

Turbulent coronal heating and the distribution of nanoflares
por: Dmitruk, P., et al.
Publicado: (1997)

Turbulent coronal heating and the distribution of nanoflares
por: Dmitruk, P., et al.

Turbulent coronal heating and the distribution of nanoflares
por: Dmitruk, P., et al.
Publicado: (1997)

Magnetohydrodynamic turbulence of coronal active regions and the distribution of nanoflares
por: Dmitruk, Pablo Ariel, et al.
Publicado: (1998)

An eruptive complex solar flare and events in its aftermath
Publicado: (2016)

An eruptive complex solar flare and events in its aftermath
por: Luoni, M.L., et al.

Turbulent coronal heating and the distribution of nanoflares
por: Dmitruk, Pablo Ariel, et al.
Publicado: (1997)

Comparison of 30 THz impulsive burst time development to microwaves, Hα, EUV, and GOES soft X-rays
por: Miteva, R., et al.

Comparison of 30 THz impulsive burst time development to microwaves, Hα, EUV, and GOES soft X-rays
Publicado: (2016)

Atmospheric heating in solar flares by chromospheric condensation
Publicado: (1994)

Atmospheric heating in solar flares by chromospheric condensation
por: Gan, W.Q., et al.

Observando la cromosfera solar en el infrarrojo
por: Giménez de Castro, C. G.
Publicado: (2023)

Multi-resolution wavelet analysis of high time resolution millimeter wavelength observations of solar bursts
Publicado: (2001)

Multi-resolution wavelet analysis of high time resolution millimeter wavelength observations of solar bursts
por: Giménez De Castro, C.G., et al.

Ultraviolet events observed in active regions. II. An interpretation of flaring arches and associated small flares
Publicado: (1997)

Ultraviolet events observed in active regions. II. An interpretation of flaring arches and associated small flares
por: Fontenla, J., et al.

A solar burst with a spectral component observed only above 100 GHz during an M class flare
Publicado: (2008)

A solar burst with a spectral component observed only above 100 GHz during an M class flare
por: Cristiani, G., et al.

Efecto Neupert: análisis para fulguraciones del Ciclo Solar 24
por: Cristiani, G., et al.
Publicado: (2024)

The white-light flare of 1982 June 15: A midchromospheric kernel
Publicado: (1993)

The white-light flare of 1982 June 15: A midchromospheric kernel
por: Mauas, P.J.D.

Chromospheric models of a solar flare including velocity fields
Publicado: (2002)

Chromospheric models of a solar flare including velocity fields
por: Falchi, A., et al.

Quasi-separatrix layers in solar flares: II. Observed magnetic configurations
Publicado: (1997)

Quasi-separatrix layers in solar flares: II. Observed magnetic configurations
por: Démoulin, P., et al.

Lack of universality in mhd turbulence, and the possible emergence of a new paradigm?
por: Mininni, Pablo Daniel
Publicado: (2010)

Lack of universality in mhd turbulence, and the possible emergence of a new paradigm?
por: Pouquet, A., et al.
Publicado: (2010)