The magnetic field configuration of a solar prominence inferred from spectropolarimetric observations in the He i 10 830 Å triplet⋆

Author： Orozco Suárez D.   Asensio Ramos A.   Trujillo Bueno J.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|566|issue|A46-A46

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.566, Iss.issue, 2014-06, pp. : A46-A46

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

Abstract

Related content

Observations of Ellerman bomb emission features in He i D3 and He i 10 830 Å⋆

By Libbrecht Tine   Joshi Jayant   Rodríguez Jaime de la Cruz   Leenaarts Jorrit   Ramos Andrés Asensio  

Astronomy & Astrophysics, Vol. 598, Iss. issue, 2017-01 ,pp. : A33-A33

Edp Sciences

Access to resources Recommend Favorite

On the formation of the He I 10 830 Å line in a flaring atmosphere

By  

Astronomy & Astrophysics, Vol. 432, Iss. 2, 2005-03 ,pp. : 699-704

Edp Sciences

Access to resources Recommend Favorite

Active cool stars and He I 10 830 Å: the coronal connection

By  

Astronomy & Astrophysics, Vol. 488, Iss. 2, 2008-09 ,pp. : 715-721

Edp Sciences

Access to resources Recommend Favorite

Spicule emission profiles observed in He i 10 830 Å

By  

Astronomy & Astrophysics, Vol. 472, Iss. 3, 2007-09 ,pp. : L51-L54

Edp Sciences

Access to resources Recommend Favorite

Multicomponent He I 10 830 Å profiles in an active filament

By Sasso C.   Lagg A.   Solanki S. K.  

Astronomy & Astrophysics, Vol. 526, Iss. issue, 2010-12 ,pp. : A42-A42

Edp Sciences

Access to resources Recommend Favorite