LEADER 04078nam 2200865z- 450 001 9910367750703321 005 20231214133345.0 010 $a3-03921-466-7 035 $a(CKB)4100000010106210 035 $a(oapen)https://directory.doabooks.org/handle/20.500.12854/44147 035 $a(EXLCZ)994100000010106210 100 $a20202102d2019 |y 0 101 0 $aeng 135 $aurmn|---annan 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aCosmic Plasmas and Electromagnetic Phenomena 210 $cMDPI - Multidisciplinary Digital Publishing Institute$d2019 215 $a1 electronic resource (264 p.) 311 $a3-03921-465-9 330 $aDuring the past few decades, plasma science has witnessed a great growth in laboratory studies, in simulations, and in space. Plasma is the most common phase of ordinary matter in the universe. It is a state in which ionized matter (even as low as 1%) becomes highly electrically conductive. As such, long-range electric and magnetic fields dominate its behavior. Cosmic plasmas are mostly associated with stars, supernovae, pulsars and neutron stars, quasars and active galaxies at the vicinities of black holes (i.e., their jets and accretion disks). Cosmic plasma phenomena can be studied with different methods, such as laboratory experiments, astrophysical observations, and theoretical/computational approaches (i.e., MHD, particle-in-cell simulations, etc.). They exhibit a multitude of complex magnetohydrodynamic behaviors, acceleration, radiation, turbulence, and various instability phenomena. This Special Issue addresses the growing need of the plasma science principles in astrophysics and presents our current understanding of the physics of astrophysical plasmas, their electromagnetic behaviors and properties (e.g., shocks, waves, turbulence, instabilities, collimation, acceleration and radiation), both microscopically and macroscopically. This Special Issue provides a series of state-of-the-art reviews from international experts in the field of cosmic plasmas and electromagnetic phenomena using theoretical approaches, astrophysical observations, laboratory experiments, and state-of-the-art simulation studies. 610 $acosmic ray knee and ankle 610 $ablazars 610 $anumerical methods 610 $aglobal jets 610 $aMHD?accretion 610 $amuti-messenger astronomy 610 $amassive star supernovae 610 $agalaxies: active 610 $aTBD 610 $a26Al 610 $ablack holes 610 $aaccreting black holes 610 $aparticle-in-cell simulations 610 $akink-like instability 610 $alaser-induced nuclear reactions 610 $amagnetic fields 610 $amagneto-hydrodynamics 610 $agamma-ray bursts 610 $aactive galactic nuclei 610 $aaccretion discs?jets 610 $anumerical relativity 610 $aplasma physics 610 $aGRMHD 610 $ahigh-power laser systems 610 $aradio interferometry 610 $arecollimation shocks 610 $aeffective lifetime 610 $amulti-wavelength astronomy 610 $arelativistic jets 610 $ahigh energy astrophysics 610 $ajets 610 $aactive galaxies 610 $arelativistic astrophysics 610 $ahelical magnetic fields 610 $alaser plasma 610 $aX-ray binaries 610 $apolarization 610 $athe Weibel instability 610 $aAGN 610 $aneutrino astrophysics 610 $aradiation mechanism: non-thermal 610 $anuclear astrophysics 610 $acosmic rays 610 $amushroom instability 610 $aaccretion disks 610 $aMHD winds 700 $aMeli$b Athina$4auth$01288170 702 $aGómez$b Jose L$4auth 702 $aMizuno$b Yosuke$4auth 906 $aBOOK 912 $a9910367750703321 996 $aCosmic Plasmas and Electromagnetic Phenomena$93020669 997 $aUNINA