Two-dimensional imaging of the development phase of plasma instabilities in the Earth's ionosphere

The convective ionospheric storm (CIS) is a naturally occurring process in the earth's ionosphere over the magnetic equator that can have deleterious consequences on satellite navigation and communication systems. By making low-elevation optical observations from Haleakala, Hawaii, the two-dime...

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Bibliographic Details
Published inIEEE transactions on plasma science Vol. 33; no. 2; pp. 502 - 503
Main Authors Makela, J.J., Kelley, M.C.
Format Journal Article
LanguageEnglish
Published New York IEEE 01.04.2005
The Institute of Electrical and Electronics Engineers, Inc. (IEEE)
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Summary:The convective ionospheric storm (CIS) is a naturally occurring process in the earth's ionosphere over the magnetic equator that can have deleterious consequences on satellite navigation and communication systems. By making low-elevation optical observations from Haleakala, Hawaii, the two-dimensional structure (2-D) (altitude versus longitude) can be made. We present observations from April 30, 2003 that clearly show the development phase of the CIS and compare them to a nonlinear simulation of the instability process. Through long-term observations of this type, we will collect a database that will be used to help unravel some of the outstanding questions associated with this fascinating phenomenon.
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ISSN:0093-3813
1939-9375
DOI:10.1109/TPS.2005.845119