The influence of small scale magnetic fields on profiles of magnetically sensitive λ 525.02 nm and λ 1564.85 nm Fe I lines in the quiet solar photosphere
Heading:
1Stodilka, MI 1Astronomical Observatory of Ivan Franko National University of Lviv, Lviv, Ukraine |
Kinemat. fiz. nebesnyh tel (Online) 2011, 27(4):3-23 |
Start Page: Solar Physics |
Language: Ukrainian |
Abstract: An analytical estimate for integral influence of small-scale magnetic fields on the line absorption co efficient is derived. The formation of the magnetically sensitive Fe I lines in the conditions of the quiet solar photosphere in the presence of small-scale magnetic fields is studied. It is shown that these fields are liable to spread wings of magnetically sensitive lines. |
Keywords: quiet solar photosphere, small scale magnetic fields |