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• W2040761712 abstract "In the present paper the quasi-static model of Landini & Monsignori Fossi ([CITE]) for coronal loops is improved and a simple diagnostic procedure is developed to compare the most important physical properties of the model with a set of spectral observations of loops such as those obtained by the CDS and SUMER instruments on SOHO. The model assumes quasi-static and isobaric conditions and solves the energy equation among radiative losses, a constant heating function and heat conduction. The model is allowed to have a variable loop section. To better match the latest observational results, an isothermal section of the loop is added at the top of the loop model; its effects on the diagnostic technique and on the shape of the unknown heating function are discussed. A numerical simulation is shown and the effect of the isothermal region is discussed. In a second paper (Brkovic et al. [CITE], Paper II) the present model will be compared with observations from the SOHO satellite." @default.
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• W2040761712 date "2002-02-01" @default.
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• W2040761712 title "Models for solar magnetic loops" @default.
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• W2040761712 doi "https://doi.org/10.1051/0004-6361:20011759" @default.
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