This thesis is a study of cosmic ray propagation within turbulent magnetic fields. Turbulent scale-lengths were altered and the behaviour of cosmic rays was observed within both large and small-scale magnetic fields, thereby giving an indication of the actual paths they may follow in space, and consequently providing some clues as to their origins.Thesis (M.Sc.) -- University of Adelaide, School of Chemistry and Physics, 200
10 pages, 17 figures, invited talk for CRIS'04 (Cosmic Ray International Seminar), May 31 - June 4 2...
Simple cosmic ray diffusion in magnetic fields is often discussed in terms of a characteristic scatt...
International audienceWe calculate the diffusion coefficients of charged cosmic rays (CR) propagatin...
In this research, the diffusion of high energy cosmic rays (protons) in turbulent magnetic fields wa...
We present a new analysis of the transport of cosmic rays in a turbulent magnetic Ðeld that varies i...
Cosmic-ray anisotropy has been observed in a wide energy range and at different angular scales by a ...
We obtain the angular distribution of the cosmic rays reaching an observer from an individual source...
Copyright © Astronomical Society of Australia 2000There is now evidence that there may be a strong s...
The magnetic fields associated with young stellar objects are expected to have an hour-glass geometr...
15 pages, 20 figuresWe extend previous studies of mixed-composition extragalactic cosmic-ray source ...
We study the diffusion of cosmic rays (CRs) in turbulent magnetic fields using test particle simulat...
The science problem I have tackled in this grant is the derivation of the diffusion tensor of energe...
[Abstract] Cosmic rays with relativeistic high energy, inner or outer the Galaxy of their origins, w...
We study the influence of the random part of the galactic magnetic field on the propagation of ultra...
To appear in the proceedings of CRIS 2004International audienceWe discuss the influence of large sca...
10 pages, 17 figures, invited talk for CRIS'04 (Cosmic Ray International Seminar), May 31 - June 4 2...
Simple cosmic ray diffusion in magnetic fields is often discussed in terms of a characteristic scatt...
International audienceWe calculate the diffusion coefficients of charged cosmic rays (CR) propagatin...
In this research, the diffusion of high energy cosmic rays (protons) in turbulent magnetic fields wa...
We present a new analysis of the transport of cosmic rays in a turbulent magnetic Ðeld that varies i...
Cosmic-ray anisotropy has been observed in a wide energy range and at different angular scales by a ...
We obtain the angular distribution of the cosmic rays reaching an observer from an individual source...
Copyright © Astronomical Society of Australia 2000There is now evidence that there may be a strong s...
The magnetic fields associated with young stellar objects are expected to have an hour-glass geometr...
15 pages, 20 figuresWe extend previous studies of mixed-composition extragalactic cosmic-ray source ...
We study the diffusion of cosmic rays (CRs) in turbulent magnetic fields using test particle simulat...
The science problem I have tackled in this grant is the derivation of the diffusion tensor of energe...
[Abstract] Cosmic rays with relativeistic high energy, inner or outer the Galaxy of their origins, w...
We study the influence of the random part of the galactic magnetic field on the propagation of ultra...
To appear in the proceedings of CRIS 2004International audienceWe discuss the influence of large sca...
10 pages, 17 figures, invited talk for CRIS'04 (Cosmic Ray International Seminar), May 31 - June 4 2...
Simple cosmic ray diffusion in magnetic fields is often discussed in terms of a characteristic scatt...
International audienceWe calculate the diffusion coefficients of charged cosmic rays (CR) propagatin...