Observations of pressure anisotropy effects within semi-collisional magnetized plasma bubbles.

Observations of pressure anisotropy effects within semi-collisional magnetized plasma bubbles.
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DOI:
10.1038/s41467-020-20387-7
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发表时间:
2021-01-12
影响因子:
16.6
通讯作者:
Woolsey NC
Woolsey NC
中科院分区:
综合性期刊1区
文献类型:
--
作者:
Tubman ER;Joglekar AS;Bott AFA;Borghesi M;Coleman B;Cooper G;Danson CN;Durey P;Foster JM;Graham P;Gregori G;Gumbrell ET;Hill MP;Hodge T;Kar S;Kingham RJ;Read M;Ridgers CP;Skidmore J;Spindloe C;Thomas AGR;Treadwell P;Wilson S;Willingale L;Woolsey NC

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Magnetized plasma interactions are ubiquitous in astrophysical and laboratory plasmas. Various physical effects have been shown to be important within colliding plasma flows influenced by opposing magnetic fields, however, experimental verification of the mechanisms within the interaction region has remained elusive. Here we discuss a laser-plasma experiment whereby experimental results verify that Biermann battery generated magnetic fields are advected by Nernst flows and anisotropic pressure effects dominate these flows in a reconnection region. These fields are mapped using time-resolved proton probing in multiple directions. Various experimental, modelling and analytical techniques demonstrate the importance of anisotropic pressure in semi-collisional, high-β plasmas, causing a reduction in the magnitude of the reconnecting fields when compared to resistive processes. Anisotropic pressure dynamics are crucial in collisionless plasmas, but are often neglected in collisional plasmas. We show pressure anisotropy to be essential in maintaining the interaction layer, redistributing magnetic fields even for semi-collisional, high energy density physics (HEDP) regimes. Magnetic fields can be reorganized by plasma flows and lead to effects such as magnetic reconnection. Here the authors explore the evolution of magnetized-plasma bubbles in a semi-collisional regime and the role of pressure anisotropy in influencing the flow of the laser-produced plasma.
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