Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kfnt...13a..50g&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, vol. 13, p. 50
Astronomy and Astrophysics
Astrophysics
Solar Magnetic Field, Solar Activity, Chromosphere, Photosphere, Magnetic Flux, Astronomical Observatories
Scientific paper
We present results of observations of longitudinal magnetic fields in two active regions on the sun. The observations were carried out in the lines Fe I 525.3 nm and H-beta by means of the double magnetograph of the Crimean Astrophysical Observatory. In our analysis, we compare the observed magnetic field with the potential field. The strong magnetic fields in the chromosphere have a smaller inclination to the vertical line than those fields in the photosphere. The difference of this inclination decreases with magnetic intensity. The observed magnetic field structure in the chromosphere differs from the potential one at the same height.
Gandzha Ivan S.
Gopasyuk O. S.
Gopasyuk S. I.
Shakhovskaya A. N.
Tarasova T. N.
No associations
LandOfFree
Comparison of observed and calculated magnetic field structures for a potential model for two active regions 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 Comparison of observed and calculated magnetic field structures for a potential model for two active regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison of observed and calculated magnetic field structures for a potential model for two active regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1605307