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- W2092498150 abstract "view Abstract Citations (29) References (40) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Interrelation of Soft and Hard X-Ray Emissions during Solar Flares. I. Observations Winglee, R. M. ; Kiplinger, A. L. ; Zarro, D. M. ; Dulk, G. A. ; Lemen, J. R. Abstract The interrelation between the acceleration and heating of electrons and ions during impulsive solar flares is determined on the basis of simulataneous observations of hard and soft X-ray emission from the Solar Maximum Mission at high time resolution (6 s). For all the flares, the hard X-rays are found to have a power-law spectrum which breaks down during the rise phase and beginning of the decay phase. After that, the spectrum changes to either a single power law or a power law that breaks up at high energies. The characteristics of the soft X-ray are found to depend on the flare position. It is suggested that small-scale quasi-static electric fields are important for determining the acceleration of the X-ray-producing electrons and the outflowing chromospheric ions. Publication: The Astrophysical Journal Pub Date: July 1991 DOI: 10.1086/170196 Bibcode: 1991ApJ...375..366W Keywords: Particle Acceleration; Solar Flares; Solar Spectra; Solar X-Rays; X Ray Spectra; Chromosphere; Doppler Effect; Solar Maximum Mission; Spectral Energy Distribution; Solar Physics; PARTICLE ACCELERATION; RADIATION MECHANISMS; SUN: FLARES; SUN: X-RAYS full text sources ADS | Related Materials (1) Part 2: 1991ApJ...375..382W" @default.
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- W2092498150 date "1991-07-01" @default.
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- W2092498150 title "Interrelation of soft and hard X-ray emissions during solar flares. I - Observations" @default.
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