Coronal Spectroscopy For Dynamo Studies

Rachel Osten
Magnetic reconnection lies at the heart of much stellar phenomena in the cool half of the H-R diagram, and X-ray studies of stellar coronae have revealed the intricate interplay of plasma and magnetic fields, ultimately produced as the result of a dynamo process. The breakthrough of Chandra and XMM-Newtons high resolution spectrometers for these stars lay in revealing the wealth of diagnostic information, used to demonstrate the structuring and energetics of hot plasma, and the...
This data repository is not currently reporting usage information. For information on how your repository can submit usage information, please see our documentation.