LEADER 02438nam0 22003853i 450 001 SUN0093351 005 20151120101600.498 100 $a20130416d2001 |0engc50 ba 101 $aeng 102 $aIT 105 $a|||| ||||| 200 1 $aSemigroups of automatic transformations$fC. K. Gupta and V. I. Sushchansky 205 $aRoma : Aracne$b2001 210 $d21 cm 215 $aEstratto da: Quaderni di matematica, n. 8 (2001), p. 203-220. 606 $aSemigroups of transformations, etc. [MSC 2010] 20M20$2MF$3SUNC023848 606 $aSemigroups in automata theory, linguistics, etc. [MSC 2010] 20M35$2MF$3SUNC028848 620 $dRoma$3SUNL000360 700 1$aGupta$b, C. K.$3SUNV074987$0722539 701 1$aSushchansky$b, V. I.$3SUNV074988$0722538 712 $aAracne$3SUNV001104$4650 801 $aIT$bSOL$c20181109$gRICA 912 $aSUN0093351 950 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08 CONS Estratto / 8 9 $e08 6096 950 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08 CONS Estratto / 8 9 $e08 6097 950 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08 CONS Estratto / 8 9 $e08 6098 950 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08 CONS Estratto / 8 9 $e08 6099 950 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08 CONS Estratto / 8 9 $e08 6100 995 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$bIT-CE0120$h6096$kCONS Estratto / 8 9$oc$qa 995 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$bIT-CE0120$h6097$kCONS Estratto / 8 9$oc$qa 995 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$bIT-CE0120$h6098$kCONS Estratto / 8 9$oc$qa 995 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$bIT-CE0120$h6099$kCONS Estratto / 8 9$oc$qa 995 $aUFFICIO DI BIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$bIT-CE0120$h6100$kCONS Estratto / 8 9$oc$qa 996 $aSemigroups of automatic transformations$91409115 997 $aUNICAMPANIA LEADER 01787nam 2200493 450 001 9910702735003321 005 20150227082241.0 035 $a(CKB)5470000002430851 035 $a(OCoLC)904125145 035 $a(EXLCZ)995470000002430851 100 $a20150227j201403 ua 0 101 0 $aeng 135 $aurcn||||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aBuckling analysis for stiffened anisotropic circular cylinders based on Sanders' nonlinear shell theory /$fMichael P. Nemeth 210 1$aHampton, Virginia :$cNational Aeronautics and Space Administration, Langley Research Center,$dMarch 2014. 215 $a1 online resource (408 pages) $ccolor illustrations 225 1 $aNASA/TM ;$v2014-218176 300 $aTitle from title screen (viewed Feb. 27, 2015). 300 $a"March 2014." 320 $aIncludes bibliographical references (pages 131-138). 606 $aNonlinear equations$2nasat 606 $aRayleigh-Ritz method$2nasat 606 $aShell theory$2nasat 606 $aShell stability$2nasat 606 $aAnisotropic shells$2nasat 606 $aDonnell equations$2nasat 615 7$aNonlinear equations. 615 7$aRayleigh-Ritz method. 615 7$aShell theory. 615 7$aShell stability. 615 7$aAnisotropic shells. 615 7$aDonnell equations. 700 $aNemeth$b Michael P.$01391721 712 02$aLangley Research Center, 712 02$aUnited States.$bNational Aeronautics and Space Administration, 801 0$bGPO 801 1$bGPO 906 $aBOOK 912 $a9910702735003321 996 $aBuckling analysis for stiffened anisotropic circular cylinders based on Sanders' nonlinear shell theory$93481438 997 $aUNINA LEADER 05440nam 22007331 450 001 9910806929603321 005 20240401173949.0 010 $a9783527656240 010 $a3527656243 010 $a9783527656226 010 $a3527656227 010 $a9783527656257 010 $a3527656251 035 $a(CKB)2550000001117150 035 $a(EBL)1388819 035 $a(OCoLC)858654466 035 $a(SSID)ssj0001154670 035 $a(PQKBManifestationID)11719283 035 $a(PQKBTitleCode)TC0001154670 035 $a(PQKBWorkID)11162799 035 $a(PQKB)10054056 035 $a(MiAaPQ)EBC1388819 035 $a(Au-PeEL)EBL1388819 035 $a(CaPaEBR)ebr10762534 035 $a(CaONFJC)MIL517588 035 $a(PPN)224991213 035 $a(Perlego)1002833 035 $a(EXLCZ)992550000001117150 100 $a20131006d2014 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aCollisionless plasmas in astrophysics /$fGerard Belmont [and four others] 205 $a1st ed. 210 1$aHoboken, New Jersey :$cJohn Wiley & sons,$d2014. 215 $a1 online resource (427 p.) 300 $aDescription based upon print version of record. 311 08$a9783527410743 311 08$a3527410740 311 08$a9781299863378 311 08$a129986337X 320 $aIncludes bibliographical references and index. 327 $aCollisionless Plasmas in Astrophysics; Contents; About the Authors; 1 Introduction; 1.1 Goals of the Book; 1.2 Plasmas in Astrophysics; 1.2.1 Plasmas Are Ubiquitous; 1.2.2 The Magnetosphere of Stars; 1.2.3 Shock Waves; 1.2.4 Planetary Magnetospheres; 1.3 Upstream of Plasma Physics: Electromagnetic Fields and Waves; 1.3.1 Electromagnetic Fields; 1.3.2 Transverse and Longitudinal Electromagnetic Field; 1.3.3 Electromagnetic Fields in Vacuum; 1.3.4 Plane Waves in a Plasma; 1.3.5 Electromagnetic Components of Plane Plasma Waves 327 $a1.3.6 Some General Properties of Plane Wave Polarization and Dispersion1.3.7 Electrostatic Waves; 1.3.8 Wave Packets and Group Velocity; 1.3.9 Propagation of Plane Waves in a Weakly Inhomogeneous Medium; 1.3.10 Useful Approximations of the Maxwell Equations in Plasma Physics; 1.4 Upstream of Plasma Physics: The Motion of Charged Particles; 1.4.1 The Motion of the Guiding Center; 1.4.2 Adiabatic Invariants; 1.4.3 The Motion of a Particle in a Wave; 2 Plasma Descriptions and Plasma Models; 2.1 Distribution Function and Moments; 2.1.1 From Individual Particles to Kinetic Description 327 $a2.1.2 Kinetic Description and First Order Moments2.1.3 Higher-Order Moments; 2.1.4 Moments for a Mixture of Populations; 2.1.5 Nontrivial Generalization of the Fluid Concepts; 2.1.6 Fluid vs. Kinetic Description: An Example; 2.2 From Kinetic to Fluid Equations; 2.2.1 Moment Equations; 2.2.2 Lagrangian Form of the Moment Equations; 2.2.3 Fluid Equations: Necessity of a Closure Equation; 2.2.4 Collisional Limit: Fluid Dynamics and Thermodynamics; 2.3 Numerical Methods; 2.3.1 Vlasov Codes; 2.3.2 Particle in Cell Codes (PIC); 2.3.3 Perturbative PIC Codes; 2.4 Fluid Codes; 2.5 Hybrid Codes 327 $a3 The Magnetized Plasmas3.1 Ideal MHD; 3.1.1 The Ideal MHD System; 3.1.2 The Ideal Ohm's Law; 3.2 Establishing the MHD Model; 3.2.1 Large-Scale Conditions of Validity; 3.2.2 Departures from MHD: Multi-Fluid and Kinetic Effects; 3.3 Dimensional Analysis and Plasma Characteristic Scales; 3.3.1 Dimensional Analysis: The General Methods; 3.3.2 Temporal and Spatial Scales, Adimensional Numbers; 3.3.3 Dispersive and Dissipative Effects; 3.3.4 Physical Importance of the Dimensionless Parameters; 4 Collisional-Collisionless; 4.1 Notion of Collisions in Plasma Physics 327 $a4.1.1 Coulomb Interaction: A Long Range Interaction4.1.2 Mean Free Path; 4.1.3 The Debye Length and the Notion of Debye "Screening"; 4.1.4 Knudsen Number; 4.1.5 Plasma Regimes; 4.2 Notion of Dissipation; 4.2.1 Transfers of Energy and Dissipation; 4.2.2 The Concept of Dissipation in Collisional Fluids; 4.2.3 Reversibility; 4.2.4 Irreversibility and Damping; 4.2.5 The Notion of Reversibility Depends on the Description; 4.2.6 Entropy; 5 Waves in Plasmas; 5.1 MHD Waves; 5.1.1 Polarization of the MHD Waves; 5.1.2 Application: Alfve?n and MHD Waves in the Earth's Magnetosphere 327 $a5.2 Transport Induced by Waves 330 $a Collisionless Plasmas in Astrophysics examines the unique properties of media without collisions in plasma physics. Experts in this field, the authors present the first book to concentrate on collisionless conditions in plasmas, whether close or not to thermal equilibrium. Filling a void in scientific literature, Collisionless Plasmas in Astrophysics explains the possibilities of modeling such plasmas, using a fluid or a kinetic framework. It also addresses common misconceptions that even professionals may possess, on phenomena such as "collisionless (Landau) damping". Abundant illustration 606 $aCollisionless plasmas 606 $aPlasma astrophysics 615 0$aCollisionless plasmas. 615 0$aPlasma astrophysics. 676 $a530.446 700 $aBelmont$b Gerard$01685554 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910806929603321 996 $aCollisionless plasmas in astrophysics$94057788 997 $aUNINA