Solar Coronal Magnetic Fields: Quantitative Measurements at Radio Wavelengths
2019
Quantitative measurements of coronal and chromospheric magnetic field is currently in its infancy. We describe a foundation of such observations, which is a key input for MHD numerical models of the solar atmosphere and eruptive processes, and a key link between lower layers of the solar atmosphere and the heliosphere.
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
0
References
0
Citations
NaN
KQI