01236nam2 22002893i 450 RML016865320231121125656.020070912d2007 ||||0itac50 baengfiz01i xxxe z01n1.:Edited by Jaako Frösén, Tiina Purola, Erja SalmenkiviHelsinkiSocietas Scientiarum Fennica2007547 p.ill.25 cm.001RML01686502001 Proceedings of the 24. International Congress of PapyrologyHelsinki, 1-7 August, 2004Edited by Jaako Frösén, Tiina Purola, Erja Salmenkivi1091Manoscritti21ITIT-0120070912IT-RM0418 IT-RM0151 IT-FR0017 BIBLIOTECA ACCADEMIA NAZ. DEI LINCEI E CORSINIANARM0418 Biblioteca Istituto Storico Italiano Medio Evo - IRM0151 Biblioteca umanistica Giorgio ApreaFR0017 RML0168653Biblioteca umanistica Giorgio Aprea 52S.SIJ. E6.ICP (24,2004) 1 52SBA0000145255 VMN RS C 2012120420121204 10 41 52161339UNICAS04513nam 22009973a 450 991036775070332120250203235429.09783039214662303921466710.3390/books978-3-03921-466-2(CKB)4100000010106210(oapen)https://directory.doabooks.org/handle/20.500.12854/44147(ScCtBLL)9927b4e5-a672-414a-bd01-f2a08d75cf77(OCoLC)1163848926(oapen)doab44147(EXLCZ)99410000001010621020250203i20192019 uu engurmn|---annantxtrdacontentcrdamediacrrdacarrierCosmic Plasmas and Electromagnetic PhenomenaAthina Meli, Yosuke Mizuno, Jose L. GómezMDPI - Multidisciplinary Digital Publishing Institute2019Basel, Switzerland :MDPI,2019.1 electronic resource (264 p.)9783039214655 3039214659 During 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.Astronomy, space & timebicssccosmic ray knee and ankleblazarsnumerical methodsglobal jetsMHD–accretionmuti-messenger astronomymassive star supernovaegalaxies: activeTBD26Alblack holesaccreting black holesparticle-in-cell simulationskink-like instabilitylaser-induced nuclear reactionsmagnetic fieldsmagneto-hydrodynamicsgamma-ray burstsactive galactic nucleiaccretion discs–jetsnumerical relativityplasma physicsGRMHDhigh-power laser systemsradio interferometryrecollimation shockseffective lifetimemulti-wavelength astronomyrelativistic jetshigh energy astrophysicsjetsactive galaxiesrelativistic astrophysicshelical magnetic fieldslaser plasmaX-ray binariespolarizationthe Weibel instabilityAGNneutrino astrophysicsradiation mechanism: non-thermalnuclear astrophysicscosmic raysmushroom instabilityaccretion disksMHD windsAstronomy, space & timeMeli Athina1288170Mizuno YosukeGómez Jose LScCtBLLScCtBLLBOOK9910367750703321Cosmic Plasmas and Electromagnetic Phenomena3020669UNINA