Studying astrophysical collisionless shocks with counterstreaming plasmas from high power lasers

Studying astrophysical collisionless shocks with counterstreaming plasmas from high power lasers

Collisions of high Mach number flows occur frequently in astrophysics, and the resulting shock waves are responsible for the properties of many astrophysical phenomena, such as supernova remnants, Gamma Ray Bursts and jets from Active Galactic Nuclei. Because of the low density of astrophysical plas...

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Bibliographic Details
Main Authors: Park, H, Ryutov, D, Ross, J, Kugland, N, Glenzer, S, Plechaty, C, Pollaine, S, Remington, B, Spitkovsky, A, Gargate, L, Gregori, G, Bell, A, Murphy, C, Sakawa, Y, Kuramitsu, Y, Morita, T, Takabe, H, Froula, D, Fiksel, G, Miniati, F, Koenig, M, Ravasio, A, Pelka, A, Liang, E, Woolsey, N
Format: Journal article
Language:English
Published: 2012

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