Abstract
Hα observations with high temporal resolution allow a detailed analysis of the chromospheric response to thre primary energy release. The timing; relationship between Hα and hard X-rays gives information about the energy transport mechanism. Sites of massive injection of nonthermal electrons are identified by characteristic features in the the line profile (Canfield et al. 1984;. Canfield and Gayley 1987).
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.