![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
Author: Yasnov L. Kal’tman T. Bogod V.
Publisher: MAIK Nauka/Interperiodica
ISSN: 1063-7729
Source: Astronomy Reports, Vol.55, Iss.1, 2011-01, pp. : 82-90
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Related content
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
Methods for deriving the magnetic field in solar (radio) active regions
By Zhao R.
Astrophysics and Space Science, Vol. 280, Iss. 3, 2002-01 ,pp. :