The importance of anisotropic interstellar turbulence and molecular-cloud magnetic mirrors for galactic cosmic-ray propagation

Space Science Reviews

Volumn 99, Issue 1-4, 2001, Pages 271-280

  Chandran, Benjamin D G ^a  

^a UNIVERSITY OF IOWA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; ASTRONOMY; CALCULATION; CONFERENCE PAPER; COSMIC RADIATION; HYDRODYNAMICS; MAGNETIC FIELD; MAGNETISM; THEORY; TURBULENT FLOW;

EID: 0035714618     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1013809502161     Document Type: Conference Paper

References (17)

1. Molecular clouds are not fractal: A characteristic size scale in Taurus
2. Cosmic-ray confinement in the Galaxy
3. Scattering of energetic particles by anisotropic magnetohydrodynamic turbulence with a goldreich-sridhar power spectrum
4. Confinement and isotropization of galactic cosmic rays by molecular-cloud magnetic mirrors when turbulent scattering is weak
5. The anisotropy of magnetohydrodynamic alfvénic turbulence
6. Intercloud structure in a turbulent fractal interstellar medium
7. A fractal origin for the mass spectrum of interstellar cloud
8. Toward a theory of interstellar turbulence. 2: Strong alfvénic turbulence
9. The IRAM key project: Small-scale structure of per-star forming regions
10. Inertial-range spectrum of hydromagnetic turbulence
11. Anisotropy in MHD turbulence due to a mean magnetic field
12. Interstellar magnetic field strengths and gas densities: Observational and theoretical perspectives
13. Observations of the magnetic fields inside and outside the Milky Way
14. Magnetic fields in galaxies and beyond