Very Large Array Faraday rotation studies of the coronal plasma
Knowledge of the coronal magnetic field is crucial for understanding (1) the heating mechanism(s) of the solar corona, (2) the acceleration of the fast solar wind, and (3) the structure and dynamics of coronal mass ejections (CMEs). Observation of Faraday rotation (FR) is one of the best remote-sens...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Others |
| Language: | English |
| Published: |
University of Iowa
2016
|
| Subjects: | |
| Online Access: | https://ir.uiowa.edu/etd/2100 https://ir.uiowa.edu/cgi/viewcontent.cgi?article=6650&context=etd |