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...
Hauptverfasser: | 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 |
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Format: | Journal article |
Sprache: | English |
Veröffentlicht: |
2012
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