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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Published in | IEEE transactions on plasma science Vol. 33; no. 2; pp. 502 - 503 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
New York
IEEE
01.04.2005
The Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
Subjects | |
Online Access | Get full text |
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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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Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 ObjectType-Article-1 ObjectType-Feature-2 |
ISSN: | 0093-3813 1939-9375 |
DOI: | 10.1109/TPS.2005.845119 |