On the magnetic quenching of mean-field effects in supersonic interstellar turbulence
On the magnetic quenching of mean-field effects in supersonic interstellar turbulence
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超音速星际湍流中平均场效应的磁猝灭
DOI：
10.1093/mnras/sts356
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发表时间：
2013
影响因子：
4.8
通讯作者：
Elstner
中科院分区：
文献类型：
--
作者：
Gressel;Bendre;Elstner
The emergence of large-scale magnetic fields observed in the diffuse interstellar medium is explained by a turbulent dynamo. The underlying transport coefficients have previously been extracted from numerical simulations. So far, this was restricted to thekinematicregime, but we aim to extend our analysis into the realm of dynamically important fields. This marks an important step on which derived mean-field models rely to explain observed equipartition-strength fields. As in previous work, we diagnose turbulent transport coefficients by means of the test-field method. We derive quenching functions for the dynamo α effect, diamagnetic pumping and turbulent diffusivity, which are compared with theoretical expectations. At late times, we observe the suppression of the vertical wind. Because this potentially affects the removal of small-scale magnetic helicity, new concerns arise about circumventing constraints imposed by the conservation of magnetic helicity at high magnetic Reynolds numbers. While present results cannot safely rule out this possibility, the issue only becomes important at late stages and is absent when the dynamo is quenched by the wind itself.
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