Einaudi, Giorgio, 1950-....
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Giorgio Einaudi astrophysicien italien
Einaudi, Giorgio
VIAF ID: 114899412 (Personal)
Permalink: http://viaf.org/viaf/114899412
Preferred Forms
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200 _ 1
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Einaudi
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, Giorgio
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200 _ |
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Einaudi
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Giorgio
‡f
1950-....
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100 1 _ ‡a Einaudi, Giorgio
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100 1 _
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Einaudi, Giorgio
(sparse)
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100 1 _
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Einaudi, Giorgio
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1950-
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100 1 _ ‡a Einaudi, Giorgio, ‡d 1950-
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100 1 0
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Einaudi, Giorgio,
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1950-
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100 1 _ ‡a Einaudi, Giorgio, ‡d 1950-
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100 1 _
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Einaudi, Giorgio,
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1950-....
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100 0 _
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Giorgio Einaudi
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astrophysicien italien
4xx's: Alternate Name Forms (2)
Works
| Title | Sources |
|---|---|
| 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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