An information-theoretical methodology for profile parameter estimation of solar coronal spectra

E-ISSN： 1432-0746|455|3|1081-1089

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.455, Iss.3, 2006-09, pp. : 1081-1089

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

Parameter estimation for a nonlinear control-oriented tokamak profile evolution model

By Geelen P Felici F Merle A Sauter O

Plasma Physics and Controlled Fusion, Vol. 57, Iss. 12, 2015-12 ,pp. : 125008-125023

IOP Publishing

Access to resources Recommend Favorite

“Ultimate” information content in solar and stellar spectra

Astronomy & Astrophysics, Vol. 492, Iss. 1, 2008-12 ,pp. : 199-213

Edp Sciences

Access to resources Recommend Favorite

Steps towards a high precision solar rotation profile: Results from SDO/AIA coronal bright point data

By Sudar D. Skokić I. Brajša R. Saar S. H.

Astronomy & Astrophysics, Vol. 575, Iss. issue, 2015-02 ,pp. : A63-A63

Edp Sciences

Access to resources Recommend Favorite

Dynamics of solar coronal loops

Astronomy & Astrophysics, Vol. 424, Iss. 1, 2004-09 ,pp. : 289-300

Edp Sciences

Access to resources Recommend Favorite

Dynamics of solar coronal loops

Astronomy & Astrophysics, Vol. 411, Iss. 3, 2003-12 ,pp. : 605-613

Edp Sciences

Access to resources Recommend Favorite