Role of E region conductivity in the development of equatorial ionospheric plasma bubbles

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dc.contributor.author Bhattacharyya, A.
dc.date.accessioned 2015-08-25T06:22:03Z
dc.date.accessioned 2021-02-12T09:27:30Z
dc.date.available 2015-08-25T06:22:03Z
dc.date.available 2021-02-12T09:27:30Z
dc.date.issued 2004
dc.identifier.citation Geophysical Research Letters, v.31/6, 2004, doi: 10.1029/2003GL018960 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/273
dc.description.abstract [1] A transmission line analogy, which has been used earlier in a linear theory for the development of equatorial plasma bubbles, is extended to study the effect of E region conductivity on non-linear evolution of the plasma bubbles. For this, a set of mode coupling equations are used to describe non-linear development of equatorial plasma bubbles in the presence of field-aligned currents which couple the equatorial F region with conjugate E regions. For a three mode system, these non-linear equations yield a condition for unstable fixed states. This condition shows that E region resistivity together with F region polariz-ability introduces another time scale in the non-linear evolution of equatorial bubbles, and this is the time scale for discharging the bubbles. en_US
dc.language.iso en en_US
dc.subject Ionospheric plasma en_US
dc.subject Plasma bubbles en_US
dc.subject Equatorial ionospheric en_US
dc.subject E region en_US
dc.title Role of E region conductivity in the development of equatorial ionospheric plasma bubbles en_US
dc.type Article en_US
dc.identifier.accession 090761


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