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- W1981781288 abstract "Abstract The data obtained at high temporal and spectral resolution with the Bent Crystal Spectrometer of the Solar Maximum Mission have shown that the soft x-ray spectra emitted by highly ionized heavy ions are characterised during the impulsive phase of flares by blue-shifted components. The blue emission has been interpreted as due to convective plasma flows from the chromosphere, which in flare conditions is heated to coronal temperatures. In the present study, the properties of the Ca XIX solar spectra are compared with the results of numerical calculations simulating the behaviour of coronal plasma subject to impulsive heating. The plasma hydrodynamic response to transient heating is modeled in the assumption of a fluid confined in a semicircular loop of uniform cross-section. Two different forms of heating are considered: direct thermal heating, and heating due to injection in the loop of non-thermal electrons." @default.
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- W1981781288 date "1986-01-01" @default.
- W1981781288 modified "2023-09-27" @default.
- W1981781288 title "Hydrodynamics of coronal loops: A comparison of observed and simulated spectra emitted from flaring coronal loops" @default.
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- W1981781288 doi "https://doi.org/10.1016/0273-1177(86)90136-5" @default.
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