A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
The Reversed Polarity Structures of Chromospheric Magnetic Fields in Active Regions
1993
International Astronomical Union Colloquium
Preserved Fulltext
AbstractThe reversed polarity structures of chromospheric magnetic fields are magnetic gulfs and islands of opposite polarity relative to the underlying photospheric fields. In this paper data were analyzed from the Solar Magnetic Field Telescope of the Huairou Solar Observing Station (HSOS) in Beijing. From more than 300 pairs of photospheric magnetograms (in FeIλ5324.19 Å) and relevant chromospheric magnetograms (in Hβλ4861.34 Å), the reality of the reversed polarity structures is
doi:10.1017/s0252921100029286
fatcat:wjad3dkdbvfn5ivkoy45l7qlxe