dc.creatorHoyos, Jaime H.
dc.creatorReisenegger Von Oepen Tassilo, Andreas
dc.creatorValdivia, Juan A.
dc.date.accessioned2022-05-16T13:00:31Z
dc.date.available2022-05-16T13:00:31Z
dc.date.created2022-05-16T13:00:31Z
dc.date.issued2011
dc.identifier10.1109/PLASMA.2011.5993219
dc.identifier9781612843292
dc.identifier0730-9244
dc.identifier9781612843308
dc.identifier0730-9244
dc.identifierhttps://ieeexplore.ieee.org/stamp/stamp.jsp?arnumber=5993219
dc.identifierhttps://doi.org/10.1109/PLASMA.2011.5993219
dc.identifierhttps://repositorio.uc.cl/handle/11534/63937
dc.description.abstractSummary form only given. We study the effect of the ambipolar diffusion (joint transport of magnetic flux and charged particles relative to neutral particles) on the long-term evolution of a magnetic field one dimensional configuration. Our system is a weakly ionized plasma in which neutral and charged particles can be converted into each other through nuclear beta decays or ionization-recombination processes. We show numerically that ambipolar diffusion tends to spread out the magnetic flux, but, contrary to the normal Ohmic diffusion, it produces sharp magnetic-field gradients with associated current sheets around those regions where the magnetic field is weak. These results could have applications in explaining relevant processes promoting the magnetic field evolution inside neutron stars (particularly magnetars), magnetic field evolution in the interstellar medium and the loss of magnetic flux from collapsing molecular cloud cores.
dc.languageen
dc.publisherIEEE
dc.relationIEEE International Conference on Plasma Science (2011 : Chicago, Estados Unidos)
dc.rightsacceso restringido
dc.subjectPlasmas
dc.titleAmbipolar diffusion in weakly ionized plasmas
dc.typecomunicación de congreso


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