Abstract
An analysis of the data of Achong and Stahl (1984) discloses discrete intervals which differ significantly in SID flare incidence and the proportion of complex sunspot groups present. This supports the alternative interpretation of Sawyer et al. (1985) in respect of the strong dependence of SID flare production on complex magnetic class.
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.
