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- W2071448995 abstract "view Abstract Citations (138) References (106) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Observed Characteristics of Flare Energy Release. I. Magnetic Structure at the Energy Release Site Machado, Marcos E. ; Moore, Ronald L. ; Hernandez, Ana M. ; Rovira, Marta G. ; Hagyard, Mona J. ; Smith, Jesse B., Jr. Abstract It is shown that flaring activity as seen in X-rays usually encompasses two or more interacting magnetic bipoles within an active region. Soft and hard X-ray spatiotemporal evolution is considered as well as the time dependence of the thermal energy content in different magnetic bipoles participating in the flare, the hardness and impulsivity of the hard X-ray emission, and the relationship between the X-ray behavior and the strength and 'observable shear' of the magnetic field. It is found that the basic structure of a flare usually consists of an initiating closed bipole plus one or more adjacent closed bipoles impacted against it. Publication: The Astrophysical Journal Pub Date: March 1988 DOI: 10.1086/166106 Bibcode: 1988ApJ...326..425M Keywords: Magnetohydrodynamics; Solar Flares; Solar Magnetic Field; Solar X-Rays; Light Curve; Magnetic Field Configurations; Magnetic Poles; Particle Acceleration; Solar Maximum Mission; Solar Physics; HYDROMAGNETICS; SUN: FLARES; SUN: X-RAYS full text sources ADS | Related Materials (1) Part 2: 1988ApJ...326..451M" @default.
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- W2071448995 date "1988-03-01" @default.
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- W2071448995 title "The observed characteristics of flare energy release. I - Magnetic structure at the energy release site" @default.
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