Formation of ionisation layers responsible for blanketing Es during daytime counter-electrojet over magnetic equator

Pandey, R. ; Prakash, S. ; Sinha, H. S. S. (1992) Formation of ionisation layers responsible for blanketing Es during daytime counter-electrojet over magnetic equator Journal of Atmospheric and Terrestrial Physics, 54 (1). pp. 63-74. ISSN 0021-9169

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Official URL: http://www.sciencedirect.com/science/article/pii/0...

Related URL: http://dx.doi.org/10.1016/0021-9169(92)90085-Y

Abstract

A model using photochemistry and transport due to electric fields and gravity wave winds has been used to explain the formation of ionisation layers observed over an equatorial station Thumba (dip 0°47′S) with rocket-borne Langmuir probes during two daytime counter-electrojet periods. These layers were seen as blanketing Es-layers with an ionosonde at Thumba. Convergence of the metallic ions due to three-dimensional gravity wave winds and a westward electric field appears to be mainly responsible for the observed ionisation layer over the equator.

Item Type:Article
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ID Code:97751
Deposited On:19 Sep 2013 11:45
Last Modified:19 Sep 2013 11:45

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