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DC Field | Value | Language |
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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 | |
Appears in Collections: | UAS_Reprints |
Files in This Item:
File | Description | Size | Format | |
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BhattacharyyaA_GRL_2004.pdf | Reprint | 85.66 kB | Adobe PDF | View/Open |
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