On determining the electron density dist
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Martin D. Altschuler; R. Michael Perry
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Article
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1972
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Springer
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English
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The electron density distribution of the inner solar corona (r ~< 2 R| as a function of latitude, longitude, and radial distance is determined from K-coronameter polarization-brightness (pB) data. A Lcgendre polynomial is assumed for the electron density distribution, and the coefficients of the pol