Abstract
The solar explosive events are further studied taking Joule dissipation and thermal conduction into account. The former heats up the plasmoid of the magnetic island, the latter cools it down. The results are consistent with S.-P. Jin's previous work that did not include either factors, and display more clearly the phenomenon of high-velocity flow in these events.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
