dc.contributor.author |
Moolla, S. |
|
dc.contributor.author |
Bharuthram, R. |
|
dc.contributor.author |
Singh, S.V. |
|
dc.contributor.author |
Lakhina, G.S. |
|
dc.date.accessioned |
2015-08-25T08:53:28Z |
|
dc.date.accessioned |
2021-02-12T10:11:11Z |
|
dc.date.available |
2015-08-25T08:53:28Z |
|
dc.date.available |
2021-02-12T10:11:11Z |
|
dc.date.issued |
2003 |
|
dc.identifier.citation |
Pramana-Journal of Physics, v.61/6, p.1209-1214, 2003, doi: 10.1007/BF02704418 |
en_US |
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/278 |
|
dc.description.abstract |
Using fluid theory, a set of equations is derived for non-linear high-frequency waves propagating oblique to an external magnetic field in a three-component plasma consisting of hot electrons, cold electrons and cold ions. For parameters typical of the Earth’s magnetosphere, numerical solutions of the governing equations yield sinusoidal, sawtooth or bipolar wave-forms for the electric field. |
en_US |
dc.language.iso |
en |
en_US |
dc.subject |
Magnetosphere |
en_US |
dc.subject |
Bipolar |
en_US |
dc.subject |
Sawtooth wave-forms |
en_US |
dc.subject |
Electric fields |
en_US |
dc.subject |
Non-linear high-frequency waves |
en_US |
dc.title |
Non-linear high-frequency waves in the magnetosphere |
en_US |
dc.type |
Article |
en_US |
dc.identifier.accession |
090767 |
|