Why are coronal holes indistinguishable from the quiet sun in transition region radiation

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 575, 2004, Pages 35-40

  Wiegelmann, Thomas ^a   Solanki, Sami K ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Coronal heating; Coronal holes; Magnetic fields; SOHO15

Indexed keywords

COMPUTER SIMULATION; MAGNETIC FIELD EFFECTS; MAGNETIC FLUX; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; SURFACE TREATMENT; TECTONICS; THERMAL EFFECTS;

CORONAL HEATING; CORONAL HOLES; SOHO 15; TRANSITION REGION;

SUN;

EID: 22144480318     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

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