Published 1971
| public
Book Section - Chapter
Application of the Chromospheric Magnetograph to Active Regions
- Creators
- Zirin, H.
- Other:
- Howard, Robert
Abstract
We show how to determine the magnetic field structure in active regions from the Ha morphology. We also show the role of the EFR (emerging flux region) as a bipolar region of velocity downflow. Finally, we point out that since all new magnetic flux emerges in strictly bipolar form, complex spot groups must result from surface interaction, hence most of the solar surface field may be produced on the surface.
Additional Information
© International Astronomical Union 1971. I am indebted to A. Bhatnagar and J. Adkins for magnetograms, and to Peter Foukal for numerous discussions. This work was supported by NASA and by the Atmospheric Sciences section of the NSF.Additional details
- Eprint ID
- 106049
- DOI
- 10.1007/978-94-010-3117-2_31
- Resolver ID
- CaltechAUTHORS:20201013-155619681
- NASA
- NSF
- Created
-
2020-10-14Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- International Astronomical Union Symposium (IAUS)
- Series Volume or Issue Number
- 43