Developed turbulence and nonlinear amplification of magnetic fields in laboratory and astrophysical plasmas. by Meinecke, J, Tzeferacos, P, Bell, A, Bingham, R, Clarke, R, Churazov, E, Crowston, R, Doyle, H, Drake, R, Heathcote, R, Koenig, M, Kuramitsu, Y, Kuranz, C, Lee, D, MacDonald, M, Murphy, C, Notley, M, Park, H, Pelka, A, Ravasio, A, Reville, B, Sakawa, Y, Wan, W, Woolsey, N, Yurchak, R, Miniati, F, Schekochihin, A, Lamb, D, Gregori, G

Polarization of thermal bremsstrahlung emission due to electron pressure anisotropy by Komarov, S, Khabibullin, I, Churazov, E, Schekochihin, A

“…Astrophysical plasmas are typically magnetized, with the Larmor radii of the charged particles many orders of magnitude smaller than their collisional mean free paths. …”

Self-inhibiting thermal conduction in a high-β, whistler-unstable plasma by Komarov, S, Schekochihin, A, Churazov, E, Spitkovsky, A

“…This result can be applied to high-β astrophysical plasmas, such as the intracluster medium, where thermal conduction at sharp temperature gradients along magnetic-field lines can be significantly suppressed. …”