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

Publisher： Edp Sciences

E-ISSN： 1432-0746|395|3|975-975

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.395, Iss.3, 2002-12, pp. : 975-975

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

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

Edp Sciences

Access to resources Recommend Favorite

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

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

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

Edp Sciences

Access to resources Recommend Favorite

UVCS/SOHO observations of a CME-driven shock: Consequences on ion heating mechanisms behind a coronal shock

By  

Astronomy & Astrophysics, Vol. 383, Iss. 1, 2002-02 ,pp. : 267-274

Edp Sciences

Access to resources Recommend Favorite

Coronal O VI emission observed with UVCS/SOHO during solar flares: Comparison with soft X-ray observations

By Mancuso S.   Giordano S.   Raymond J. C.  

Astronomy & Astrophysics, Vol. 591, Iss. issue, 2016-06 ,pp. : A4-A4

Edp Sciences

Access to resources Recommend Favorite

UVCS/SOHO investigation of the interface between streamers and coronal holes

By  

Astronomy & Astrophysics, Vol. 429, Iss. 1, 2005-01 ,pp. : 353-360

Edp Sciences

Access to resources Recommend Favorite