Day-to-day variability of the equatorial electrojet strength

Kane, R.P.; Trivedi, N.B.; Tanaka, Y.; Hajime, Y.; Pathan, B.M.

dc.contributor.author	Kane, R.P.
dc.contributor.author	Trivedi, N.B.
dc.contributor.author	Tanaka, Y.
dc.contributor.author	Hajime, Y.
dc.contributor.author	Pathan, B.M.
dc.date.accessioned	2015-09-22T11:05:19Z
dc.date.accessioned	2021-02-12T09:25:15Z
dc.date.available	2015-09-22T11:05:19Z
dc.date.available	2021-02-12T09:25:15Z
dc.date.issued	2003
dc.identifier.citation	Indian Journal of Radio and Space Physics, v.32, p.251-260, 2003	en_US
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/469
dc.description.abstract	The H ranges at the equatorial electrojet locations Ancon, Peru and Trivandrum, India, show substantial periodicities in the 2-20 day range which are absent in solar flux , and hence, should be attributed mainly to planetary wave activity and more so in quiet-sun intervals. However, the results for the two locations differ in details, indicating that these effects may not be global. The variations are seen mostly in the daytime values, indicating their association with the daytime electrojet strength only.	en_US
dc.language.iso	en	en_US
dc.subject	Equatorial electrojet	en_US
dc.subject	Magnetic field component	en_US
dc.subject	Electrojet	en_US
dc.subject	Planetary wave	en_US
dc.title	Day-to-day variability of the equatorial electrojet strength	en_US
dc.type	Article	en_US
dc.identifier.accession	090976