Addendum to: Strength of the Solar Coronal Magnetic Field - A Comparison of Independent Estimates Using Contemporaneous Radio and White-Light Observations
DOI: 10.1007/s11207-017-1203-3
Bibcode: 2017SoPh..292..177K
Kumari, Anshu; Ramesh, R.; Kathiravan, C.; Wang, T. J.
India, United States
Abstract
This addendum uses an alternate fit for the electron density distribution N (r ) (see Figure 1) and estimates the coronal magnetic field using the new model. We find that the estimates of the magnetic field are in close agreement using both the models.
2017
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Solar Physics
SOHO
11