UVCS/SOHO observations of a CME-driven shock: Consequences on ion heating mechanisms behind a coronal shock

Astronomy and Astrophysics

Volumn 383, Issue 1, 2002, Pages 267-274

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

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

Author keywords

Magnetohydrodynamics (MHD); Shock waves; Sun: corona, UV radiation, radio radiation

Indexed keywords

DOPPLER EFFECT; IONS; LIGHT EMISSION; MAGNETOHYDRODYNAMICS; PROTONS; SHOCK WAVES; SOLAR RADIATION; SPECTROMETRY; SUN; ULTRAVIOLET RADIATION;

CORONAL MASS EJECTION (CME); CORONAL SHOCKS;

ASTROPHYSICS;

EID: 0036473455     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20011721     Document Type: Article

References (30)