Generation of scaled protogalactic seed magnetic fields in laser-produced shock waves.

The standard model for the origin of galactic magnetic fields is through the amplification of seed fields via dynamo or turbulent processes to the level consistent with present observations. Although other mechanisms may also operate, currents from misaligned pressure and temperature gradients (the...

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Những tác giả chính:	Gregori, G, Ravasio, A, Murphy, C, Schaar, K, Baird, A, Bell, A, Benuzzi-Mounaix, A, Bingham, R, Constantin, C, Drake, R, Edwards, M, Everson, E, Gregory, C, Kuramitsu, Y, Lau, W, Mithen, J, Niemann, C, Park, H, Remington, B, Reville, B, Robinson, A, Ryutov, D, Sakawa, Y, Yang, S, Woolsey, N
Định dạng:	Journal article
Ngôn ngữ:	English
Được phát hành:	2012

Generation of scaled protogalactic seed magnetic fields in laser-produced shock waves.

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