Addendum to: Strength of the Solar Coronal Magnetic Field - A Comparison of Independent Estimates Using Contemporaneous Radio and White-Light Observations
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.
- Publication:
-
Solar Physics
- Pub Date:
- December 2017
- DOI:
- 10.1007/s11207-017-1203-3
- Bibcode:
- 2017SoPh..292..177K
- Keywords:
-
- Solar Coronal Magnetic Field;
- White-light Observations;
- Independent Estimates;
- Coronal Mass Ejections (CME);
- Fifth-order Polynomial