Imaging large scale plasma disturbances in the inner heliosphere

Details Imaging large scale plasma disturbances in the inner heliosphere Imaging large scale plasma disturbances in the inner heliosphere

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994r%26qe...37..339h&link_type=abstract

Radiophysics and Quantum Electronics, Volume 37, Issue 5, pp.339-343

Physics

Scientific paper

Many radiogalaxies scintillate due to density variations in the solar wind. By observing large numbers of radio galaxies on a regular daily basis scintillation can be used to map the structure and movement of major disturbances in the solar wind between the Sun and the Earth. Such global information about “weather patterns” in the solar wind adds an important new dimension to space research and aids the interpretation of in situ observations from spacecraft. The observational method is described and some new insights into solar-terrestrial physics are discussed.

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