Zobrazeno 1 - 10
of 177
pro vyhledávání: '"Russell M. Kulsrud"'
Autor:
Eve C. Ostriker
Publikováno v:
Physics Today. 59:58-58
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d901934c86a28fb16e03996db4bedbe8
https://doi.org/10.1063/1.2180179
https://doi.org/10.1063/1.2180179
Most of the theoretical results on the kinematic amplification of small-scale magnetic fluctuations by turbulence have been confined to the model of white-noise-like advecting turbulent velocity field. In this work, the statistics of the passive magn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ee8ed4b98d0be3f279ccdf88a0fd80cc
https://doi.org/10.1063/1.1404383
https://doi.org/10.1063/1.1404383
Autor:
Russell M. Kulsrud, Alexander Schekochihin, Steven Cowley, Gregory W. Hammett, Prateek Sharma
We show that under very general conditions, cluster plasmas threaded by weak magnetic fields are subject to very fast growing plasma instabilities driven by the anisotropy of the plasma pressure (viscous stress) with respect to the local direction of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cfdebf989d6632fbb6743ee2a9af9eb
https://doi.org/10.1086/431202
https://doi.org/10.1086/431202
Autor:
Russell M. Kulsrud
Publikováno v:
AIP Conference Proceedings.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::025f82b0061a1a3a4887e04dfe80886d
https://doi.org/10.1063/1.4944013
https://doi.org/10.1063/1.4944013
Autor:
Russell M. Kulsrud
Publikováno v:
Journal of Plasma Physics. 81
In previous galactic dynamo theories of the origin of the magnetic field in our galaxy, the subject of flux-freezing has been omitted. As a consequence, the equation of mass flow has generally also been omitted, particularly in the halo where the gal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c02cb11c676878fce5256df34040382f
https://doi.org/10.1017/s0022377815001397
https://doi.org/10.1017/s0022377815001397
Publikováno v:
Astrophysics and Space Science. 298:219-226
A short summary of recent progress in measuring and understanding turbulence during magnetic reconnection in laboratory plasmas is given. Magnetic reconnection is considered as a primary process to dissipate magnetic energy in laboratory and astrophy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::99c4040c18ca4faa6151e4437baf21ba
https://doi.org/10.1007/s10509-005-3936-y
https://doi.org/10.1007/s10509-005-3936-y
Publikováno v:
Physics of Plasmas. 10:319-322
Measurement of the transverse resistivity was carried out in a reconnecting current sheet where the mean free path for the Coulomb collision is smaller than the thickness of the sheet. In a collisional neutral sheet without a guide field, the transve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d4275f8b11f4d2de3bf159481013ab17
https://doi.org/10.1063/1.1528612
https://doi.org/10.1063/1.1528612
Autor:
Russell M. Kulsrud
Publikováno v:
Earth, Planets and Space. 53:417-422
The two theories for magnetic reconnection, one of Sweet and Parker, and the other of Petschek, are reconciled by exhibiting an extra condition in that of Petschek which reduces his theory to that of Sweet and Parker, provided that the resistivity is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b2a5bff039bff335118285920f584af
https://doi.org/10.1186/bf03353251
https://doi.org/10.1186/bf03353251
Autor:
Russell M. Kulsrud, Leonid Malyshkin
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 316:249-266
We consider the possibility of time variations of the solar neutrino flux due to the radial motion of the Earth and neutrino interference effects. We calculate the time variations of the detected neutrino flux and the extent to which they are suppres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8bb6fa75b48a4a25493d5c14e950684
https://doi.org/10.1046/j.1365-8711.2000.03522.x
https://doi.org/10.1046/j.1365-8711.2000.03522.x
Publikováno v:
Scopus-Elsevier
During magnetic reconnection, a “neutral sheet” current is induced, heating the plasma. The resultant plasma thermal pressure forms a stationary equilibrium with the opposing magnetic fields. The reconnection layer profile holds significant clues
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6209987f8156c5c650655d1de31c61e2
https://doi.org/10.1063/1.873999
https://doi.org/10.1063/1.873999