Zobrazeno 1 - 10
of 133
pro vyhledávání: '"R.M. Kulsrud"'
Autor:
R.M. Kulsrud
Publikováno v:
Astronomische Nachrichten. 331:22-26
A serious difficulty with the standard alpha-omega theory of the origin of galactic magnetic fields involves the question of flux expulsion. This is intimately related to flux freezing. The alpha-omega theory is shown in the context of the giant supe
Autor:
R.M. Kulsrud, R.R. Rafikov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 314:839-848
The possibility of the magnetic flux expulsion from the Galaxy in the superbubble (SB) explosions, important for the Alpha-Omega dynamo, is considered. Special emphasis is put on the investigation of the downsliding of the matter from the top of the
Autor:
R.M. Kulsrud, G.M. Felice
The authors study the problem of cosmic ray diffusion in the galactic disk with particular attention to the problem of particle scattering through the {theta} = cos{sup {minus}1} ({nu}{sub {parallel}}/{nu}) = 90{degree} pitch angle in momentum space
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::52161652b8f4df080a02c02797d8a06e
https://doi.org/10.2172/764465
https://doi.org/10.2172/764465
Local ion temperature is measured directly in the well-characterized reconnection layer of a laboratory plasma. These measurements demonstrate definitively that ions are heated due to reconnection and that more than half of the reconnected field ener
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d4e2068982e221f5ebaac142efbd2948
https://doi.org/10.2172/14732
https://doi.org/10.2172/14732
Autor:
R.M. Kulsrud, D.A. Uzdensky
We study the two-dimensional global scale magnetic field structure for a system of two merging cylindrical plasmas in a steady state. In the limit of very large magnetic Reynolds numbers the reconnection process is slow, and the plasma almost everywh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::48e4cc2969fad4d37ff09ece02140379
https://doi.org/10.2172/293436
https://doi.org/10.2172/293436