Abstract
Using a 1995–2000 data set of vector magnetograms from the Huairou Solar Observing Station(HSOS) of National Astronomical Observatory, the magnetic shear angles of 311 active regions(908 vector magnetograms) were calculated. It is found that the statistical distribution of the magnetic shear angles can be fitted well by Gaussian curves. The chirality of the solar magnetic fields was analyzed using the fitted distribution. The dominant chirality (the sign of the magnetic shear angles) was varied from 1995 to 2000.
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.
