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Growing electrostatic modes in the isothermal pair plasma of the pulsar magnetosphere

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dc.contributor.authorU. A., Mofiz
dc.contributor.authorAmin, Md. Ruhul
dc.contributor.authorShukła, Padma Kant
dc.contributor.departmentDepartment of Mathematics and Natural Sciences
dc.date.accessioned2016-12-06T10:26:41Z
dc.date.available2016-12-06T10:26:41Z
dc.date.issued2012
dc.descriptionThis article was published in the Astrophysics and Space Science [© 2011 Springer Science+Business Media B.V.] and the definite version is available at : http://dx.doi.org/10.1007/s10509-011-0845-0. The Journal's website is at: http://link.springer.com/article/10.1007%2Fs10509-011-0845-0en_US
dc.description.abstractIt is shown that a strongly magnetized isothermal pair plasma near the surface of a pulsar supports low-frequency (in comparison to electron cyclotron frequency) toroidal electrostatic plasma modes in the equatorial region. Physically, the thermal pressure coupled with the magnetic pressure creates the low frequency oscillations which may grow for particular case of inhomogeneities of the equilibrium magnetic field and the pair plasma density.en_US
dc.description.versionPublished
dc.identifier.citationMofiz, U. A., Amin, M. R., & Shukla, P. K. (2012). Growing electrostatic modes in the isothermal pair plasma of the pulsar magnetosphere. Astrophysics and Space Science, 337(1), 177-184. doi:10.1007/s10509-011-0845-0en_US
dc.identifier.doihttp://dx.doi.org/10.1007/s10509-011-0845-0
dc.identifier.issn0004640X
dc.identifier.urihttp://hdl.handle.net/10361/7134
dc.language.isoenen_US
dc.publisher© 2011 Springer Science+Business Media B.V.en_US
dc.subjectElectrostatic modeen_US
dc.subjectPair plasmaen_US
dc.subjectPulsar magnetosphereen_US
dc.titleGrowing electrostatic modes in the isothermal pair plasma of the pulsar magnetosphereen_US
dc.typeArticleen_US

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