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Waves In Space Plasmas (WISP)Waves in space plasmas (WISP) utilizes powerful radio transmitters and sensitive receivers to probe the secrets of the magnetosphere, ionosphere and atmosphere. The scientific objective is to achieve a better understanding of the physical processes occurring in these regions. For example, audio frequency radio waves will be radiated from the long WISP antenna, will travel to the outer reaches of the magnetosphere, and will interact with Van Allen belt particles, releasing some of their energy which amplifies the waves. Study of this interaction will give a better understanding of a major magnetospheric process, wave-particle interactions. Radio waves from WISP at higher frequencies (AM radio and beyond) will be reflected by the ionosphere and will, for example, advance our understanding of bubbles in the equatorial ionosphere which affect satellite communications.
Document ID
19860009884
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Taylor, W. W. L.
(TRW, Inc. Redondo Beach, CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1986
Publication Information
Publication: NASA. George C. Marshall Space Flight Center Solar Terrestrial Observatory Space Station Workshop Report
Subject Category
Spacecraft Instrumentation
Accession Number
86N19355
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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