LEADER 01823oam 2200505 450 001 9910709688603321 005 20180521105012.0 035 $a(CKB)5470000002471347 035 $a(OCoLC)573173276$z(OCoLC)662599079$z(OCoLC)988824701 035 $a(OCoLC)995470000002471347 035 $a(EXLCZ)995470000002471347 100 $a20100325d1927 ua 0 101 0 $aeng 135 $aur||||||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aStabilization $ehearings before the Committee on Banking and Currency, House of Representatives, Sixty-Ninth Congress, first session, on H.R. 7895 a bill to amend papragraph (d) of section 14 of the Federal Reserve Act, as amended, to provide for the stabilization of the price level for commodities in general 210 1$aWashington :$cUnited States Government Printing Office,$d1927. 215 $a1 online resource (1145 pages) $cillustrations 327 $apt. 1. March 24-25, 30-31, April 1, 6, 8-9, 12-14, 1926 -- pt. 2. April 20-22, 27, 30, May 3-6, June 10, 1926, and February 4, 1927. 517 $aStabilization 606 $aCurrency question$zUnited States 606 $aPrice maintenance$zUnited States 606 $aCurrency question$2fast 606 $aPrice maintenance$2fast 607 $aUnited States$2fast 608 $aLegislative hearings.$2lcgft 615 0$aCurrency question 615 0$aPrice maintenance 615 7$aCurrency question. 615 7$aPrice maintenance. 801 0$bOCLCE 801 1$bOCLCE 801 2$bOCLCQ 801 2$bOCLCF 801 2$bOCLCO 801 2$bOCLCQ 801 2$bZ5A 801 2$bOCLCA 801 2$bGPO 906 $aBOOK 912 $a9910709688603321 996 $aStabilization$93448528 997 $aUNINA LEADER 04513nam 22009973a 450 001 9910367750703321 005 20250203235429.0 010 $a9783039214662 010 $a3039214667 024 8 $a10.3390/books978-3-03921-466-2 035 $a(CKB)4100000010106210 035 $a(oapen)https://directory.doabooks.org/handle/20.500.12854/44147 035 $a(ScCtBLL)9927b4e5-a672-414a-bd01-f2a08d75cf77 035 $a(OCoLC)1163848926 035 $a(oapen)doab44147 035 $a(EXLCZ)994100000010106210 100 $a20250203i20192019 uu 101 0 $aeng 135 $aurmn|---annan 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 00$aCosmic Plasmas and Electromagnetic Phenomena$fAthina Meli, Yosuke Mizuno, Jose L. Gómez 210 $cMDPI - Multidisciplinary Digital Publishing Institute$d2019 210 1$aBasel, Switzerland :$cMDPI,$d2019. 215 $a1 electronic resource (264 p.) 311 08$a9783039214655 311 08$a3039214659 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. 606 $aAstronomy, space & time$2bicssc 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 $aMHD winds 615 7$aAstronomy, space & time 700 $aMeli$b Athina$01288170 702 $aMizuno$b Yosuke 702 $aGómez$b Jose L 801 0$bScCtBLL 801 1$bScCtBLL 906 $aBOOK 912 $a9910367750703321 996 $aCosmic Plasmas and Electromagnetic Phenomena$93020669 997 $aUNINA