Magnetic structure of the solar transition region as observed in various ultraviolet lines emitted at different temperatures

Publisher： Edp Sciences

E-ISSN： 1432-0746|457|2|699-706

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.457, Iss.2, 2006-10, pp. : 699-706

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Power halo and magnetic shadow in a solar quiet region observed in the Hα line

By Kontogiannis I.   Tsiropoula G.   Tziotziou K.  

Astronomy & Astrophysics, Vol. 510, Iss. issue, 2010-02 ,pp. : A41-A41

Edp Sciences

Access to resources Recommend Favorite

Temporal variability in the Doppler-shift of solar transition region lines

By  

Astronomy & Astrophysics, Vol. 396, Iss. 1, 2002-12 ,pp. : 255-267

Edp Sciences

Access to resources Recommend Favorite

Diagnostics of the κ-distribution using Si III lines in the solar transition region

By Dzifčáková E.   Kulinová A.  

Astronomy & Astrophysics, Vol. 531, Iss. issue, 2011-06 ,pp. : A122-A122

Edp Sciences

Access to resources Recommend Favorite

Emission of solar chromospheric and transition region features related to the underlying magnetic field

By Barczynski K.   Peter H.   Chitta L. P.   Solanki S. K.  

Astronomy & Astrophysics, Vol. 619, Iss. issue, 2018-10 ,pp. : A5-A5

Edp Sciences

Access to resources Recommend Favorite