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Magnetic Diffusion in Star Formation      MHD  turbulence  waves  stars  formation  ISM  clouds  ISM  magnetic fields       font style='font-size:12px;'> 2010/11/10
Magnetic diffusion plays a vital role in star formation. We trace its influence from interstellar cloud scales down to star-disk scales. On both scales, we find that magnetic diffusion can be signific...
Context. The source spectrum of cosmic rays is not well determined by diffusive shock acceleration models. The prop-agated fluxes of proton, helium, and heavier primary cosmic-ray species (up to Fe) a...
Parker instability arises from the presence of magnetic fields in a plasma such as the interstellar medium (ISM),wherein the magnetic buoyant pressure expels the gas and causes the gas to move along t...
Cosmic Ray transport in curved background magnetic fields is investigated using numerical Monte-Carlo simulation techniques. Special emphasis is laid on the So-lar system, where the curvature of the m...
Ambipolar diffusion in superfluid neutron stars     Solar and Stellar Astrophysics (astro-ph.SR)       font style='font-size:12px;'> 2010/12/24
In this paper we reconsider the problem of magnetic field diffusion in neutron star cores. We model the star as consisting of a mixture of neutrons, protons and electrons, and allow for particle react...
The propagation of high-energy cosmic rays through giant molecular clouds constitutes a fundamental process in astronomy and astrophysics. The diffusion of cosmic-rays through these magnetically turbu...
The propagation of high-energy cosmic rays through giant molecular clouds constitutes a fundamental process in astronomy and astrophysics. The diffusion of cosmic-rays through these magnetically turbu...
Atomic t tauri disk winds heated by ambipolar diffusion     Atomic t tauri disk winds  ambipolar diffusion       font style='font-size:12px;'> 2009/6/10
Atomic t tauri disk winds heated by ambipolar diffusion
Chemical Diffusion in Stellar Convective Regions     Chemical Diffusion  Stellar Convective Regions       font style='font-size:12px;'> 2009/6/10
Chemical Diffusion in Stellar Convective Regions。
Neutron diffusion and nucleosynthesis in an inhomogeneous big bang model。

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