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The Alfven-Carlquist double-layer theory of solar flares

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dc.contributor.author Hasan, S. S
dc.contributor.author Ter Haar, D
dc.date.accessioned 2009-08-28T14:39:26Z
dc.date.available 2009-08-28T14:39:26Z
dc.date.issued 1978-06
dc.identifier.citation Astrophysics and Space Science, Vol. 56, No. 1, pp. 89 - 107 en
dc.identifier.issn 0004-640X
dc.identifier.uri http://hdl.handle.net/2248/4771
dc.description.abstract We use the Vlasov equations for ions and electrons to develop a theory of a double layer in which there are both free and trapped electrons and ions. We find the equations which replace the Langmuir condition and the Bohm conditions and by numerically solving the resultant differential equation we find for particular choices of distribution functions the potential distribution in the layer. We discuss the applicability of this theory to solar flares, and show that conditions in solar flares may be such that double layers can exist for which the free particles have a power-law energy distribution. These particles will be accelerated in a double layer and may in this way account for the production of high-energy particles during the impulsive phase of solar flares. en
dc.language.iso en en
dc.publisher Kluwer Academic Publishers en
dc.relation.uri http://dx.doi.org/10.1007/BF00643464 en
dc.relation.uri http://adsabs.harvard.edu/abs/1978Ap%26SS..56...89H en
dc.rights © Kluwer Academic Publishers en
dc.subject Magnetically Trapped Particles en
dc.subject Magnetohydrodynamic Waves en
dc.subject Plasma Layers en
dc.subject Solar Flares en
dc.subject Ion Density (Concentration) en
dc.subject Solar Electrons en
dc.subject Solar Protons en
dc.subject Vlasov Equations en
dc.title The Alfven-Carlquist double-layer theory of solar flares en
dc.type Article en


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