Generation of Alfvén waves in magnetized plasma by laser plasma bunches at Mach numbers much less than unity

IF 0.6 Q4 GEOCHEMISTRY & GEOPHYSICS Solar-Terrestrial Physics Pub Date : 2022-06-30 DOI:10.12737/stp-82202214
V. Tishchenko, A. Berezutsky, Leila Dmitrieva, I. Miroshnichenko, I. Shaikhislamov
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Abstract

In this paper, we examine a torsional Alfvén wave produced by periodic plasma bunches in a magnetized plasma flux tube. A new effect has been revealed: the wave is generated not only during the action of bunches, but also for a long time after the termination, which makes it possible to increase the wavelength by several times. We have determined the conditions under which the wave contains η~40 % of the total bunch energy. The wave radius depends on the energy of one bunch; and the length, on their number. The optimum number of bunches is 15. Simultaneously with the Alfvén wave, a bunch plasma jet (η~35 %) and a slow magnetosonic wave (η~10 %) propagate in the force tube. Similarity parameters scale the results to laboratory and near-Earth magnetized plasma.
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马赫数远小于1的激光等离子体束在磁化等离子体中产生Alfvén波
本文研究了磁化等离子体磁通管内周期性等离子体束产生的扭转alfvsamn波。发现了一种新的效应:波不仅在束的作用过程中产生,而且在终止后很长一段时间内也会产生,这使得波长增加几倍成为可能。我们已经确定了波含有η~ 40%总束能量的条件。波的半径取决于一束的能量;长度,在它们的数字上。最佳的束数是15束。与alfvsamn波同时,一束等离子体射流(η~ 35%)和慢磁声波(η~ 10%)在力管中传播。相似参数将结果扩展到实验室和近地磁化等离子体。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Solar-Terrestrial Physics
Solar-Terrestrial Physics GEOCHEMISTRY & GEOPHYSICS-
CiteScore
1.50
自引率
9.10%
发文量
38
审稿时长
12 weeks
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