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Flare Emission Observed In High Resolution And Comparison With Numerical Modeling, Nengyi Huang
Flare Emission Observed In High Resolution And Comparison With Numerical Modeling, Nengyi Huang
Dissertations
As one of the most intense activities on the solar surface, flares have been extensively observed and studied ever since the first report. The standard model of solar flares has been established and commonly accepted. However, many limitations from the researching tools have left some of the problems unsolved or controversial. For example, the density of electrons in the corona is lower than it is required to activate the observed emission in HXR, and the mechanism that these electron beams can penetrate down to lower chromosphere is unclear. Many theoretical scenarios were suggested, and more observations had been in need. …