Plasma properties above coronal active regions inferred from SOHO/UVCS and radio spectrograph observations

Astronomy and Astrophysics

Volumn 400, Issue 1, 2003, Pages 347-353

  Mancuso, S ^a,b   Raymond, J C ^b   Kohl, J ^b   Ko, Y K ^b   Uzzo, M ^b   Wu, R ^b  

^a OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Shock waves; Sun: Corona; Sun: Magnetic fields; Sun: Radio radiation; Sun: UV radiation

Indexed keywords

CARRIER CONCENTRATION; ESTIMATION; MAGNETIC FIELDS; MATHEMATICAL MODELS; PLASMAS; SHOCK WAVES; SPECTROGRAPHS; SPECTROMETERS; SUN; ULTRAVIOLET RADIATION;

RADIO SPECTROGRAPHS; SOLAR CYCLE; ULTRAVIOLET CORONAGRAPH SPECTROMETER;

ASTROPHYSICS;

EID: 0037336083     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021844     Document Type: Article

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