Predictions for the propagations of energetic particles from the sun to the Earth: Influence of the magnetic turbulence

Physics and Chemistry of the Earth, Part C: Solar, Terrestrial and Planetary Science

Volumn 26, Issue 8, 2001, Pages 595-599

  Zimbardo, G ^a   Pommois, P ^a   Veltri, P ^a  

^a UNIVERSITY OF CALABRIA   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

COMMUNICATION SYSTEMS; DIFFUSION; EARTH (PLANET); HELIOGRAPHS; MAGNETOSPHERE; MONTE CARLO METHODS; NAVIGATION; SPACECRAFT;

ENERGETIC PARTICLES;

SUN;

PARTICLE MOTION; SOLAR ACTIVITY;

EID: 0034874612     PISSN: 14641917     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1464-1917(01)00053-8     Document Type: Article

References (16)

1. Energy densities of Alfvén waves between 0.7 and 1.6 AU
2. A model for the three-dimensional magnetic field correlation spectra of low-frequency solar wind fluctuations during Alfvénic periods
3. Properties of magnetohydrodynamic turbulence in the solar wind as observed by Ulysses at high heliographic latitude
4. The rate of turbulent evolution over the sun's poles
5. Stochastic aspects of magnetic lines of force with application to cosmic-ray propagation
6. Scaling laws of test particle transport in two-dimensional turbulence
7. Dynamics of the interplanetary gas and mag netic field
8. Detection of a solar particle event at an heliolatitude of 73.8°S
9. Magnetic field line transport in three dimensional turbulence: Lévy random walk and spectrum models
10. Anomalous and Gaussian transport regimes in anisotropic 3-D magnetic turbulence
11. Field line diffusion in the solar wind magnetic turbulence and energetic particle propagation across heliographic latitudes
12. Kubo number and the magnetic field line diffusion coefficient for anisotropic magnetic turbulence
13. Model of the formation of the low-latitude boundary layer for strongly northward interplanetary magnetic field
14. Electron heating in quasi-perpendicular shocks: A Monte Carlo simulation
15. Anomalous diffusion and Lévy random walk of magnetic field lines in three dimensional turbulence
16. Anomalous, quasilinear, and percolative regimes for magnetic-field-line transport in axially symmetric turbulence