Comparing eclipse observations of the 2008 August 1 solar corona with an MHD model prediction

Astronomy and Astrophysics

Volumn 513, Issue 8, 2010, Pages

  Rusin V ^a   Druckmuller M ^b   Aniol, P ^c   Minarovjech, M ^a   Saniga, M ^a   Mikic Z ^d   Linker, J A ^d   Lionello, R ^d   Riley, P ^d   Titov, V S ^d  

^a ASTRONOMICAL INSTITUTE   (Slovakia)

^b BRNO UNIVERSITY OF TECHNOLOGY   (Czech Republic)

^c ASTELCO Systems GmbH   (Germany)

^d PREDICTIVE SCIENCE INC   (United States)

Author keywords

Magnetic fields; Magnetohydrodynamics (MHD); Sun: corona

Indexed keywords

BANDPASS FILTERS; MAGNETIC FIELDS; SOLAR RADIATION;

CORONAL HEATING; CORONAL HOLE; ENERGY FORMULATIONS; MORPHOLOGICAL PROPERTIES; PASS-BAND FILTERS; POSITION ANGLE; RADIATIVE LOSS; SUN : CORONA;

MAGNETOHYDRODYNAMICS;

EID: 77952983282     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913169     Document Type: Article

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