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instabilité à coude

M=1 instability

sciences naturelles et appliquées - iate.europa.eu

kink instability

sciences naturelles et appliquées - iate.europa.eu

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Kink instability suppression with stochastic cooling pickup and kickerThe kink instability is one of the major beam dynamics issues of the linac-ring based electron ion collider....

général - core.ac.uk - PDF: digital.library.unt.edu

Relationship of the multimode kink instability to . . .We study the current-driven kink instability with a three-dimensional MHD spectral code, under conditions appropriate for the convection zone of the Sun....

PDF: citeseerx.ist.psu.edu

Kink instability: evolution and energy dissipation in relativistic force-free nonrotating jets...209200.pdf (publisher's version ) (Open Access)We study the evolution of kink instability in a force-free, nonrotating plasma column of high magnetization....

PDF: repository.ubn.ru.nl

Kink instability and stabilization of the friedmann universe with scalar fields... kink instability develops in the flatFRW universe with massless scalar fields....

PDF: arxiv.org

Kink instability and stabilization of the friedmann universe with scalar fields ...i.e., kink instability develops in the flat FRW universe with massless scalar fields....

wriggling instability

sciences naturelles et appliquées - iate.europa.eu

Publications scientifiques

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Fedrow_ott_gr21_poster.pdf... For rapid precollapse rotation resulting in protoneutron stars spinning at millisecond periods, we find the development of an m=1 instability that drives nonaxisymmetry and dramatically enhances the gravitational wave emission....

général - core.ac.uk - PDF: figshare.com

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Nonlinear evolution of the m=1 internal kink mode in the presence of magnetohydrodynamic turbulence... While the amplitudes are still small, the fastgrowing high-m TTMs enhance the growth of the m=1 instability....

général - core.ac.uk - PDF: arxiv.org

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Molecular gas and dust in ngc4550: a galaxy with two counterrotating stellar disks... The distribution of the dust and gas in the center could be the result of an m=1 instability, which is the fastest growing unstable mode in counterrotating stellar disks....

général - core.ac.uk - PDF: core.ac.uk