Addendum to: Strength of the Solar Coronal Magnetic Field - A Comparison of Independent Estimates Using Contemporaneous Radio and White-Light Observations
Published in Solar Physics, Volume 292, Issue 12, article id.177, 3 pp., 2017
Authors: Kumari, A., Ramesh, R., Kathiravan, C. & Wang, J. T.
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.
Recommended citation: Kumari, A., Ramesh, R., Kathiravan, C., and Wang, T. J., “Addendum to: Strength of the Solar Coronal Magnetic Field - A Comparison of Independent Estimates Using Contemporaneous Radio and White-Light Observations”, Solar Physics, vol. 292, no. 12, 2017. doi:10.1007/s11207-017-1203-3.