Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere

The noncollisional interaction between conducting obstacles and magnetized plasma winds can be found in different scenarios, from the interaction occurring between regions inside galaxy clusters to the interaction between the solar wind and Mars, Venus, and active comets, or even the interaction bet...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	Romanelli, N., Gómez, D., Bertucci, C., Delva, M.
Formato:	JOUR
Materias:	conduction magnetohydrodynamics (MHD) plasmas
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v789_n1_p_Romanelli
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere
por: Romanelli, Norberto Julio, et al.
Publicado: (2014)

Evidence for nonlinear development of magnetohydrodynamic scale intermittency in the inner heliosphere
por: Dmitruk, Pablo Ariel
Publicado: (2012)

Evidence for nonlinear development of magnetohydrodynamic scale intermittency in the inner heliosphere
por: Greco, A., et al.
Publicado: (2012)

Evidence for nonlinear development of magnetohydrodynamic scale intermittency in the inner heliosphere
por: Greco, A., et al.

Evidence for nonlinear development of magnetohydrodynamic scale intermittency in the inner heliosphere
por: Greco, A., et al.
Publicado: (2012)

Magnetohydrodynamic stellar wind solutions in curved magnetic fields
por: Rotstein, N.O., et al.

Magnetohydrodynamic stellar winds: A new class of solutions
por: Rotstein, N.O., et al.

Magnetohydrodynamic stellar winds: A new class of solutions
Publicado: (1995)

Magnetohydrodynamic stellar wind solutions in curved magnetic fields
Publicado: (1995)

Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: An application to the intracluster medium
por: Nakwacki, Maria Soledad
Publicado: (2014)

Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: An application to the intracluster medium
por: Santos-Lima, R., et al.
Publicado: (2014)

Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: An application to the intracluster medium
por: Santos-Lima, R., et al.

Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: An application to the intracluster medium
por: Santos-Lima, R., et al.
Publicado: (2014)

A STEADY-STATE PICTURE of SOLAR WIND ACCELERATION and CHARGE STATE COMPOSITION DERIVED from A GLOBAL WAVE-DRIVEN MHD MODEL
por: Vasquez, Alberto Marcos, et al.
Publicado: (2015)

A STEADY-STATE PICTURE of SOLAR WIND ACCELERATION and CHARGE STATE COMPOSITION DERIVED from A GLOBAL WAVE-DRIVEN MHD MODEL
por: Oran, R., et al.

Magnetohydrodynamic flows of conducting liquids in divergent-convergent channels
por: Gnavi, Graciela Delia, et al.
Publicado: (2003)

Magnetohydrodynamic flows of conducting liquids in divergent-convergent channels
por: Gnavi, G., et al.

Propagación de ondas magnetohidrodinámicas en medios magnéticamente estructurados
por: Capettini Croatto, Hilario Gabriel
Publicado: (2020)

Propagación de ondas magnetohidrodinámicas en medios magnéticamente estructurados
por: Capettini Croatto, Hilario Gabriel
Publicado: (2020)

Coronal heating by surface Alfvén wave damping: Implementation in a global magnetohydrodynamics model of the solar wind
por: Vasquez, Alberto Marcos
Publicado: (2012)

Coronal heating by surface Alfvén wave damping: Implementation in a global magnetohydrodynamics model of the solar wind
por: Evans, R.M., et al.
Publicado: (2012)

Coronal heating by surface Alfvén wave damping: Implementation in a global magnetohydrodynamics model of the solar wind
por: Evans, R.M., et al.

Coronal heating by surface Alfvén wave damping: Implementation in a global magnetohydrodynamics model of the solar wind
por: Evans, R.M., et al.
Publicado: (2012)

Turbulencia Hall-MHD en un campo magnético fuerte
por: Martín, Luis N.
Publicado: (2013)

Turbulencia Hall-MHD en un campo magnético fuerte
por: Martín, Luis N.
Publicado: (2013)

Turbulencia Hall-MHD en un campo magnético fuerte
por: Martín, Luis N.
Publicado: (2013)

Parallel simulations of hall-Mhd plasmas
por: Gómez, D.

Magnetohydrodynamical leaky waves in a layered plasma
por: González, Alejandro Guillermo, et al.
Publicado: (1998)

Magnetohydrodynamical leaky waves in a layered plasma
por: González, A.G., et al.

Test Particle Energization and the Anisotropic Effects of Dynamical MHD Turbulence
Publicado: (2017)

Test Particle Energization and the Anisotropic Effects of Dynamical MHD Turbulence
por: González, C.A., et al.

Magnetohydrodynamics /
por: Cowling, T. G. (Thomas George)
Publicado: (1957)

Alfvén waves and wings in Hall magnetohydrodynamics
por: Sallago, Patricia Alejandra, et al.
Publicado: (2004)

Hall effect in a strong magnetic field: Direct comparisons of compressible magnetohydrodynamics and the reduced Hall magnetohydrodynamic equations
por: Martin, L.N., et al.

Magnetohydrodynamics in solar and space physics
por: Gómez, D., et al.

Hall magnetohydrodynamics in a strong magnetic field
por: Gomez, Daniel Osvaldo, et al.
Publicado: (2008)

Hall effect in a strong magnetic field: Direct comparisons of compressible magnetohydrodynamics and the reduced Hall magnetohydrodynamic equations
por: Dmitruk, Pablo Ariel, et al.
Publicado: (2010)

Hall magnetohydrodynamics in a strong magnetic field
por: Gómez, D.O., et al.

Parallel simulations of hall-Mhd plasmas
Publicado: (2006)

An introduction to magnetohydrodynamics /
por: Davidson, P. A. (Peter Alan), 1957-
Publicado: (2001)