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

dc.contributor.authorBhattacharyya, A.
dc.date.accessioned2015-08-25T06:22:03Z
dc.date.accessioned2021-02-12T09:27:30Z
dc.date.available2015-08-25T06:22:03Z
dc.date.available2021-02-12T09:27:30Z
dc.date.issued2004
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.identifier.accession090761
dc.identifier.citationGeophysical Research Letters, v.31/6, 2004, doi: 10.1029/2003GL018960en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/273
dc.language.isoenen_US
dc.subjectIonospheric plasmaen_US
dc.subjectPlasma bubblesen_US
dc.subjectEquatorial ionosphericen_US
dc.subjectE regionen_US
dc.titleRole of E region conductivity in the development of equatorial ionospheric plasma bubblesen_US
dc.typeArticleen_US

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
BhattacharyyaA_GRL_2004.pdf
Size:
85.66 KB
Format:
Adobe Portable Document Format
Description:
Reprint

License bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
license.txt
Size:
1.71 KB
Format:
Plain Text
Description:

Collections