Open AccessThe solar corona above active regions: A comparison of extreme ultraviolet line emission with radio emission
Author(s) -
W. M. Neupert
Publication year - 1967
Publication title -
solar physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.026
H-Index - 123
eISSN - 1573-093X
pISSN - 0038-0938
DOI - 10.1007/bf00147845
Subject(s) - physics , extreme ultraviolet , astrophysics , sunspot , solar flare , corona (planetary geology) , flare , ultraviolet , coronal radiative losses , line (geometry) , electron temperature , electron density , ionization , radiation , coronal loop , nanoflares , emission spectrum , astronomy , coronal mass ejection , electron , spectral line , plasma , solar wind , magnetic field , optics , ion , laser , geometry , mathematics , quantum mechanics , astrobiology , venus
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