Einaudi, Giorgio, 1950-....
Giorgio Einaudi astrophysicien. - En poste, Dipartimento di fisica, Università di Pisa, Italie (en 1996)
Einaudi, Giorgio
VIAF ID: 114899412 (Personal)
Permalink: http://viaf.org/viaf/114899412
Preferred Forms
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200 _ 1 ‡a Einaudi ‡b , Giorgio
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200 _ | ‡a Einaudi ‡b Giorgio ‡f 1950-....
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100 1 _ ‡a Einaudi, Giorgio (sparse)
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100 1 _ ‡a Einaudi, Giorgio ‡d 1950-
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100 1 0 ‡a Einaudi, Giorgio, ‡d 1950-
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100 1 _ ‡a Einaudi, Giorgio, ‡d 1950-....
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100 0 _ ‡a Giorgio Einaudi ‡c astrophysicien. - En poste, Dipartimento di fisica, Università di Pisa, Italie (en 1996)
4xx's: Alternate Name Forms (2)
Works
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Alfven waves and shock wave formation at an X-point magnetic field configuration |
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The compressible evolution of the super-Alfvénic magnetized wake |
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Cyclotron instabilities of a magnetized electron plasma with anisotropic temperatures / [by] C. Chiuderi, G. Einaudi and R. Giachetti |
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Dependence of coronal loop temperature on loop length and magnetic field strength |
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Effect of pressure gradients and line-tying on the magnetic stability of coronal loops |
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Energy release in a turbulent corona |
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Field lines twisting in a noisy Corona: implications for energy storage and release, and initiation of solar eruptions |
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Hydrodynamics of the hot component of the galactic halo. II. Radiative and dynamical instabilities |
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Ideal kink instabilities in line-tied coronal loops |
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Microscale structures on the quiet sun and coronal heating |
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Modeling the Galactic Center nonthermal filaments as magnetized wakes |
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Nonlinear dynamics of the Parker scenario for coronal heating |
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Nonlinear magnetohydrodynamic evolution of line-tied coronal loops |
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Observational signatures of coronal loop heating and cooling driven by footpoint shuffling |
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Plasma astrophysics, 1996: |
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Plasmoid formation and acceleration in the solar streamer belt |
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Shear photospheric forcing and the origin of turbulence in coronal loops |
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A simplified numerical model of coronal energy dissipation based on reduced MHD |
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Statistical properties of magnetic activity in the solar Corona |
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Turbulent coronal heating mechanisms: coupling of dynamics and thermodynamics |
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