Magnetic structure of the solar transition region as observed in various ultraviolet lines emitted at different temperatures

Astronomy and Astrophysics

Volumn 457, Issue 2, 2006, Pages 699-706

  Marsch, E ^a   Zhou, G Q ^b   He, J S ^b   Tu, C Y ^a,b  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b PEKING UNIVERSITY   (China)

Author keywords

Sun: Atmosphere; Sun: Corona; Sun: Magnetic fields; Sun: Photosphere; Sun: Transition region; Sun: UV radiation

Indexed keywords

SUN: ATMOSPHERE; SUN: CORONA; SUN: MAGNETIC FIELDS; SUN: TRANSITION REGION; SUN: UV RADIATION;

EXTRATERRESTRIAL ATMOSPHERES; MAGNETIC FIELD EFFECTS; MAGNETIC STORAGE; PLASMAS; SOLAR SYSTEM; ULTRAVIOLET RADIATION;

ASTROPHYSICS;

EID: 33749640681     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065665     Document Type: Article

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