Open magnetic flux tubes in the corona and the transport of solar energetic particles

Astronomy and Astrophysics

Volumn 486, Issue 2, 2008, Pages 589-596

  Klein, K L ^a   Krucker, S ^b   Lointier, G ^a,c   Kerdraon, A ^a  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c LPCE CNRS   (France)

Author keywords

Sun: corona; Sun: flares; Sun: magnetic fields; Sun: particle emission; Sun: radio radiation; Sun: solar terrestrial relations

Indexed keywords

ATOMS; CRYSTALLOGRAPHY; ELECTRON BEAMS; EXTRAPOLATION; MAGNETIC BUBBLES; MAGNETIC DEVICES; MAGNETIC DOMAINS; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC MATERIALS; MAGNETIC STRUCTURE; MAGNETISM; PARTICLE BEAMS; RADIO ASTRONOMY; SOLAR ENERGY; SOLAR SYSTEM; SPACECRAFT; TUBES (COMPONENTS); WIND POWER;

ACTIVE REGION (AR); ECLIPTIC PLANE; ENERGETIC ELECTRONS; ENERGETIC PARTICLES; FIELD LINES; FLUX TUBES; HELIOCENTRIC ANGLE; INTERPLANETARY SPACE; LANGMUIR WAVES; LOW ENERGY ELECTRON BEAMS; MAGNETIC (CE); MAGNETIC FIELD EXTRAPOLATIONS; MAGNETIC FIELD MODELING; MAGNETIC FLUX TUBES; OPEN FIELD LINES; PARKER SPIRAL; RADIO SOURCES; SOLAR ENERGETIC PARTICLES (SEP); WIND SPACECRAFT;

INTERPLANETARY SPACECRAFT;

EID: 47249089960     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079228     Document Type: Article

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