Hot prominence detected in the core of a coronal mass ejection: Analysis of SOHO/UVCS Lα and SOHO/LASCO visible-light observations

Author： Heinzel P.   Susino R.   Jejčič S.   Bemporad A.   Anzer U.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|589|issue|A128-A128

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.589, Iss.issue, 2016-04, pp. : A128-A128

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

Context. The paper deals with the physics of erupting prominences in the core of coronal mass ejections (CME).

Related content

Hot prominence detected in the core of a coronal mass ejection

By Jejčič S.   Susino R.   Heinzel P.   Dzifčáková E.   Bemporad A.   Anzer U.  

Astronomy & Astrophysics, Vol. 607, Iss. issue, 2017-11 ,pp. : A80-A80 (NaN)

Edp Sciences

Access to resources Recommend Favorite

Hot prominence detected in the core of a coronal mass ejection

By Susino R.   Bemporad A.   Jejčič S.   Heinzel P.  

Astronomy & Astrophysics, Vol. 617, Iss. issue, 2018-09 ,pp. : A21-A21 (NaN)

Edp Sciences

Access to resources Recommend Favorite

Plasma properties above coronal active regions inferred from SOHO/UVCS and radio spectrograph observations

By  

Astronomy & Astrophysics, Vol. 400, Iss. 1, 2003-03 ,pp. : 347-353 (7)

Edp Sciences

Access to resources Recommend Favorite

UV line intensity and flow velocity distributions in two coronal mass ejections as deduced by UVCS-SOHO observations

By  

Astronomy & Astrophysics, Vol. 383, Iss. 3, 2002-03 ,pp. : 1032-1048 (17)

Edp Sciences

Access to resources Recommend Favorite

UV line intensity and flow velocity distributions in two coronal mass ejections as deduced by UVCS-SOHO observations

By  

Astronomy & Astrophysics, Vol. 395, Iss. 3, 2002-12 ,pp. : 975-975 (1)

Edp Sciences

Access to resources Recommend Favorite