Physics
Scientific paper
Mar 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981acasn..22...35s&link_type=abstract
Acta Astronomica Sinica, vol. 22, Mar. 1981, p. 35-43. In Chinese, with abstract in English.
Physics
3
Atmospheric Heating, Chromosphere, Faculae, H Alpha Line, Solar Magnetic Field, Turbulent Heat Transfer, Data Correlation, Magnetic Field Configurations, Solar Activity Effects, Solar Atmosphere, Solar Flares, Solar Physics
Scientific paper
According to the ZFM law by which chromospheric magnetic field can be derived, the paper analyzes the fine chromospheric photographs, obtained by Purple Mountain Observatory in November 1979, and study the relations among the plage, solar flare, magnetic field, wave turbulence and morphological development in H-alpha. The coupling equations for the flow-wave fields are applied to solve the problem of perpendicular heating of faculae. It is found that the narrow and long bright filament in the plage might be the feature showing horizontal heating.
Song Mu-Tao
Zhu Zhong-Yuan
No associations
LandOfFree
Analysing the magnetic structure in Hale 16398 region by the H-alpha feature and turbulent heating of plage does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Analysing the magnetic structure in Hale 16398 region by the H-alpha feature and turbulent heating of plage, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysing the magnetic structure in Hale 16398 region by the H-alpha feature and turbulent heating of plage will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1785768