Physics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...12l&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, Jan.-Feb. 1992, p. 12-19. In Russian.
Physics
6
Atmospheric Models, Magnetic Measurement, Solar Atmosphere, Solar Magnetic Field, Solar Spectra, Line Spectra, Magnetic Field Configurations, Runge-Kutta Method, Spectral Line Width
Scientific paper
The effect of anomalous dispersion on results of measurements of magnetic fields on the sun using the line-ratio method is analyzed on the basis of calculations of the Stokes parameters for the Fe I 524.7 and 525.0 nm lines and the Holveger-Mueller model atmosphere. It is shown that, with the present-day accuracy of observation data, anomalous dispersion should be taken into account only when the following conditions are simultaneously fulfilled: (1) the magnetic field slope angle exceeds 20 deg; (2) the magnetic field strength is greater than 100 mT; (3) the flux-tube magnetic profile is rectangular; and (4) the parts of the spectral line profile close to the line center (Delta lambda of less than 4 pm) are used.
Lozitskii V. G.
Sheminova V. A.
No associations
LandOfFree
The effect of anomalous dispersion in the solar atmosphere on results of magnetic field measurements using the line-ratio method 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 The effect of anomalous dispersion in the solar atmosphere on results of magnetic field measurements using the line-ratio method, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The effect of anomalous dispersion in the solar atmosphere on results of magnetic field measurements using the line-ratio method will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1049736