Intensity profiles in fluxtubes.

Bibcode
1987PAICz..66..261S
Sánchez Almeida, J.; Solanki, S. K.; Collados, M.; Del Toro Iniesta, J. C.
Bibliographical reference

Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences, No. 66, p. 261 - 263

Advertised on:
0
1987
Number of authors
4
IAC number of authors
0
Citations
0
Refereed citations
0
Description
Spectroscopic analysis of the light coming from an atmosphere is a powerful tool for revealing its properties. The problem when using conventional spectroscopy for solar fluxtubes is their unresolved character: magnetic and non-magnetic regions of a plage have to be observed as a whole. With the aim of obtaining the true intensity spectrum of an unresolved tube, the authors have developed a simple method which can reconstruct the intensity generated in the magnetic component. Only observed parameters are used: intensity and circular polarization in the plage and intensity in the quiet photosphere.
Type
Non-refereed

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