Abstract
Quantitative data on solar facalae that are a known time-varying excess brightness are presented. It is shown that facalae can produce a sufficient flux excess at the extreme solar limb so as to give a large apparent solar oblateness that can fluctuate from day to day. 13 references. (BJG)
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.
