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- W2016072247 abstract "It has been recently proposed that the solar corona is heated via the superposition of a large number of tiny energy-release events, the so-called nanoflares. In this paper we develop a simple semi-analytical model to describe the temporal evolution of the nanoflare plasma, confined in rigid magnetic flux tubes and subject to typical nanoflare energy releases. Assuming a power law for the nanoflare energy distribution and hypothesizing the repeated occurrence of nanoflares at random time intervals in an originally cool, low pressure loop, we show how a high temperature, high pressure plasma eventually builds up, leading to a nanoflare-heated corona. Even if the feasibility of the nanoflare mechanism as a coronal heating agent is thus demonstrated, we conclude by pointing out that present instrumentaiton cannot provide a definitive observational test of this hypothesis." @default.
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- W2016072247 date "1994-04-01" @default.
- W2016072247 modified "2023-09-26" @default.
- W2016072247 title "A quasi-steady model of a microflare-heated corona" @default.
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- W2016072247 doi "https://doi.org/10.1016/0273-1177(94)90174-0" @default.
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