Abstract
In the previous chapters we have considered the properties of individual flux tubes and their dynamics due to interaction with the surrounding medium. The solar atmosphere, however, consists of ensembles of flux tubes randomly distributed in space and over their parameters. In this chapter we shall consider the time-dependent response of a randomly magnetized medium to propagation of acoustic waves and unsteady wave packets. We will see that the collective phenomena resulted from these interactions lead to clear morphological effects that are observable. The character of these effects, and the associated energy input and distribution, crucially depend on the magnetic filling factor of the medium and several other factors that will be specified.
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Appendix
Appendix
To perform the integration in (6.129) we introduce the function
and change the variable \(\zeta -\zeta ' = x\). Then the double integral in (6.129) becomes (we need only its real part):
Now, the shortest way to integrate (6.143) is to use the definition of the \(\delta \)-function, namely
Therefore, (6.143) can be written as
which gives immediately
Substituting (6.146) into (6.143) we come to expression (6.130)
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Ryutova, M. (2015). Collective Phenomena in Rarefied Ensembles of Flux Tubes. In: Physics of Magnetic Flux Tubes. Astrophysics and Space Science Library, vol 417. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-45243-1_6
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DOI: https://doi.org/10.1007/978-3-662-45243-1_6
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