NDLI: Influences of the solar incidents on the Ionosphere

Content Provider	IEEE Xplore Digital Library
Author	Unver, O. Can, Z.
Copyright Year	2011
Description	Author affiliation: Yildiz Technical University, Physics Department, Istanbul/Turkey (Unver, O.; Can, Z.)
Abstract	The outmost layer of the atmosphere is called Ionosphere. This region is a natural plasma which is formed by the ionized molecules by high energy radiation comes from Sun. So, the content of the Ionosphere are made up of by the positive ions and free electrons. Content of the free electrons is called as Total Electron Content (TEC) and this is expressed by the number of free electrons on a cylinder which has one meter square cross sectional area. This electron content which is free in the ionosphere is highly effective on the radio signals that emits from earth or comes from space. The signal path varies according to the amount of the electrons. Starting from these dynamics, the predictions according to the Ionospheric TEC values could be made by looking to the affects of the electromagnetic signals, emitted from the GNSS (Global Navigation Satellite System) network, and to the delay of the duration time to reach the receiver. In this study, the influences of the solar incidents on the TEC variations have been examined.
Starting Page	593
Ending Page	597
File Size	707280
Page Count	5
File Format	PDF
ISBN	9781424496174
e-ISBN	9781424496167
DOI	10.1109/RAST.2011.5966907
Language	English
Publisher	Institute of Electrical and Electronics Engineers, Inc. (IEEE)
Publisher Date	2011-06-09
Publisher Place	Turkey
Access Restriction	Subscribed
Rights Holder	Institute of Electrical and Electronics Engineers, Inc. (IEEE)
Subject Keyword	TEC Ionization Indexes Sun Ionosphere Global Positioning System
Content Type	Text
Resource Type	Article

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Variability of TEC at mid latitude with solar activity during the solar cycle 23 and 24

Investigation of the annual solar eclipse by using Total Electron Content (TEC) measurements

Solar flare effects on the ionosphere

Ionosphereic TEC change analysis in response to solar eclipse on July $22^{nd},$ 2009

The ionospheric response to the annular solar eclipse on $26^{th}$ January 2009

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GPS Ionospheric Scintillation and Total Electron Content during partial solar eclipse in Malaysia

Short timescale variations in ionosphere caused by irregular solar electromagnetic radiation

Variations of ionospheric TEC at geomagnetic conjugate points during solar minimum

Influences of the solar incidents on the Ionosphere

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