The scalability of the accretion column in magnetic cataclysmic variables: the POLAR project
É. Falize(Centre National de la Recherche Scientifique), С. А. Пикуз(Joint Institute for High Temperatures), H. Takabe(Institute for Laser Technology), C. Grégory(Centre National de la Recherche Scientifique), C. Michaut(Observatoire de Paris), N. C. Woolsey(University of York), Yasuhiro Kuramitsu(The University of Osaka), Y. Sakawa(The University of Osaka), A. Ravasio(École Polytechnique), J.-P. Leidinger, Cécile Cavet(Centre National de la Recherche Scientifique), T. Morita(The University of Osaka), X. Ribeyre(Centre National de la Recherche Scientifique), B. Loupias(École Polytechnique), P. Barroso(Centre National de la Recherche Scientifique), A. Dizière, W. Nazarov(University of St Andrews), J. Breil(Centre National de la Recherche Scientifique)
Cited by 21
Related Papers
Self-consistent growth rate of the Rayleigh–Taylor instability in an ablatively accelerating plasma
|The Physics of Fluids|1985|505
Observation of magnetic field generation via the Weibel instability in interpenetrating plasma flows
|Nature Physics|2015|307
Nanosecond formation of diamond and lonsdaleite by shock compression of graphite
|Nature Communications|2016|251
Beat-wave excitation of plasma wave and observation of accelerated electrons
|Physical Review Letters|1992|216