LEADER 02875nam 2200673 450 001 9910791092303321 005 20230912162917.0 010 $a1-118-80849-5 010 $a1-118-80844-4 035 $a(CKB)2550000001189701 035 $a(EBL)1599322 035 $a(SSID)ssj0001174006 035 $a(PQKBManifestationID)11760923 035 $a(PQKBTitleCode)TC0001174006 035 $a(PQKBWorkID)11105993 035 $a(PQKB)10017508 035 $a(Au-PeEL)EBL1599322 035 $a(CaPaEBR)ebr10829796 035 $a(CaONFJC)MIL568626 035 $a(OCoLC)874146472 035 $a(Au-PeEL)EBL7147528 035 $a(CaSebORM)9781118808498 035 $a(MiAaPQ)EBC1599322 035 $a(MiAaPQ)EBC7147528 035 $a(EXLCZ)992550000001189701 100 $a20140205h20142014 uy 0 101 0 $aeng 135 $aurunu||||| 181 $ctxt 182 $cc 183 $acr 200 14$aThe five practices of exemplary leadership $eUnited Kingdom /$fJames M. Kouzes, Barry Z. Posner 205 $a1st edition 210 1$aSan Francisco, California :$cThe Leadership Challenge,$d2014. 210 4$d©2014 215 $a1 online resource (24 p.) 225 1 $aJ-B Leadership Challenge: Kouzes/Posner 300 $aDescription based upon print version of record. 311 $a1-118-55637-2 311 $a1-306-37375-1 327 $aCover; Copyright; Leadership Is Everyone's Business; 1. Model the Way; 2. Inspire a Shared Vision; 3. Challenge the Process; 4. Enable Others to Act; 5. Encourage the Heart; Profiles in Leadership; Claire Owen; Lance Burn; Learning to Lead; The Leadership Challenge Story; About the Authors; The Five Practices and Ten Commitments of Exemplary Leadership®; Endorsements 330 $aThis 20-page article is perfect for leaders with limited time and budget. It provides a concise overview of Kouzes and Posner's model and overall thoughts on leadership in The United Kingdom. Ideal for orienting readers to the Five Practices® model at the beginning of a workshop or coaching session, the piece contains two Leadership Challenge case studies drawn from UK nationals, a short description of the Five Practices®, a section on ""Learning to Lead"", and background information on the Leadership Practices Inventory (LPI). 410 0$aJ-B Leadership Challenge: Kouzes/Posner 606 $aLeadership 606 $aLeadership$zGreat Britain 606 $aManagement$zGreat Britain 615 0$aLeadership. 615 0$aLeadership 615 0$aManagement 676 $a658.40920941 700 $aKouzes$b James M.$f1945-$0115270 701 $aPosner$b Barry Z$0857988 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910791092303321 996 $aThe five practices of exemplary leadership$93737257 997 $aUNINA LEADER 05453nam 2200673 a 450 001 9910830659903321 005 20230617041811.0 010 $a1-280-52015-9 010 $a9786610520152 010 $a3-527-60365-4 010 $a3-527-60500-2 035 $a(CKB)1000000000377342 035 $a(EBL)481652 035 $a(OCoLC)68618374 035 $a(SSID)ssj0000195455 035 $a(PQKBManifestationID)11157108 035 $a(PQKBTitleCode)TC0000195455 035 $a(PQKBWorkID)10131293 035 $a(PQKB)10522443 035 $a(MiAaPQ)EBC481652 035 $a(EXLCZ)991000000000377342 100 $a20040827d2004 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 14$aThe magnetic universe$b[electronic resource] $egeophysical and astrophysical dynamo theory /$fGu?nther Ru?diger and Rainer Hollerbach 210 $aWeinheim $cWiley-VCH$dc2004 215 $a1 online resource (346 p.) 300 $aDescription based upon print version of record. 311 $a3-527-40409-0 320 $aIncludes bibliographical references and index. 327 $aThe Magnetic Universe Geophysical and Astrophysical Dynamo Theory; Contents; Preface; 1 Introduction; 2 Earth and Planets; 2.1 Observational Overview; 2.1.1 Reversals; 2.1.2 Other Time-Variability; 2.2 Basic Equations and Parameters; 2.2.1 Anelastic and Boussinesq Equations; 2.2.2 Nondimensionalization; 2.3 Magnetoconvection; 2.3.1 Rotation or Magnetism Alone; 2.3.2 Rotation and Magnetism Together; 2.3.3 Weak versus Strong Fields; 2.3.4 Oscillatory Convection Modes; 2.4 Taylor's Constraint; 2.4.1 Taylor's Original Analysis; 2.4.2 Relaxation of Ro = E = 0 327 $a2.4.3 Taylor States versus Ekman States2.4.4 From Ekman States to Taylor States; 2.4.5 Torsional Oscillations; 2.4.6 ??-Dynamos; 2.4.7 Taylor's Constraint in the Anelastic Approximation; 2.5 Hydromagnetic Waves; 2.6 The Inner Core; 2.6.1 Stewartson Layers on C; 2.6.2 Nonaxisymmetric Shear Layers on C; 2.6.3 Finite Conductivity of the Inner Core; 2.6.4 Rotation of the Inner Core; 2.7 Numerical Simulations; 2.8 Magnetic Instabilities; 2.9 Other Planets; 2.9.1 Mercury, Venus and Mars; 2.9.2 Jupiter's Moons; 2.9.3 Jupiter and Saturn; 2.9.4 Uranus and Neptune; 3 Differential Rotation Theory 327 $a3.1 The Solar Rotation3.1.1 Torsional Oscillations; 3.1.2 Meridional Flow; 3.1.3 Ward's Correlation; 3.1.4 Stellar Observations; 3.2 Angular Momentum Transport in Convection Zones; 3.2.1 The Taylor Number Puzzle; 3.2.2 The ?-Effect; 3.2.3 The Eddy Viscosity Tensor; 3.2.4 Mean-Field Thermodynamics; 3.3 Differential Rotation and Meridional Circulation for Solar-Type Stars; 3.4 Kinetic Helicity and the DIV-CURL-Correlation; 3.5 Overshoot Region and the Tachocline; 3.5.1 The NIRVANA Code; 3.5.2 Penetration into the Stable Layer; 3.5.3 A Magnetic Theory of the Solar Tachocline 327 $a4 The Stellar Dynamo4.1 The Solar-Stellar Connection; 4.1.1 The Phase Relation; 4.1.2 The Nonlinear Cycle; 4.1.3 Parity; 4.1.4 Dynamo-related Stellar Observations; 4.1.5 The Flip-Flop Phenomenon; 4.1.6 More Cyclicities; 4.2 The ?-Tensor; 4.2.1 The Magnetic-Field Advection; 4.2.2 The Highly Anisotropic ?-Effect; 4.2.3 The Magnetic Quenching of the ?-Effect; 4.2.4 Weak-Compressible Turbulence; 4.3 Magnetic-Diffusivity Tensor and ?-Quenching; 4.3.1 The Eddy Diffusivity Tensor; 4.3.2 Sunspot Decay; 4.4 Mean-Field Stellar Dynamo Models; 4.4.1 The ?(2)-Dynamo; 4.4.2 The ??-Dynamo for Slow Rotation 327 $a4.4.3 Meridional Flow Influence4.5 The Solar Dynamo; 4.5.1 The Overshoot Dynamo; 4.5.2 The Advection-Dominated Dynamo; 4.6 Dynamos with Random ?; 4.6.1 A Turbulence Model; 4.6.2 Dynamo Models with Fluctuating ?-Effect; 4.7 Nonlinear Dynamo Models; 4.7.1 Malkus-Proctor Mechanism; 4.7.2 ?-Quenching; 4.7.3 Magnetic Saturation by Turbulent Pumping; 4.7.4 ?-Quenching; 4.8 ?-Quenching and Maunder Minimum; 5 The Magnetorotational Instability (MRI); 5.1 Star Formation; 5.1.1 Molecular Clouds; 5.1.2 The Angular Momentum Problem; 5.1.3 Turbulence and Planet Formation 327 $a5.2 Stability of Differential Rotation in Hydrodynamics 330 $aMagnetism is one of the most pervasive features of the Universe, with planets, stars and entire galaxies all having associated magnetic fields. All of these fields are generated by the motion of electrically conducting fluids, the so-called dynamo effect. The precise details of what drives the motion, and indeed what the fluid consists of, differ widely though. In this work the authors draw upon their expertise in geophysical and astrophysical MHD to explore some of these phenomena, and describe the similarities and differences between different magnetized objects. They also explain why magn 606 $aDynamo theory (Cosmic physics) 606 $aCosmic magnetic fields 606 $aMagnetohydrodynamics 606 $aAstrophysics 615 0$aDynamo theory (Cosmic physics) 615 0$aCosmic magnetic fields. 615 0$aMagnetohydrodynamics. 615 0$aAstrophysics. 676 $a523.0188 676 $a523.01886 700 $aRu?diger$b G$g(Gu?nther)$052846 701 $aHollerbach$b Rainer$01635024 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910830659903321 996 $aThe magnetic universe$93982410 997 $aUNINA LEADER 00770nam a2200229 i 4500 001 991004379436807536 005 20250506223650.0 008 250506s1991 it af er 001 0bita d 020 $a8835501709 040 $aBibl. Dip.le Aggr. Studi Umanistici - Sez. Filosofia$bita$cSocioculturale Scs 041 1 $aita$hfre 082 04$a194$223 100 1 $aEribon, Didier$0162155 240 10$aMichel Foucault : (1926-1984)$94373873 245 10$aMichel Foucault /$cDidier Eribon ; traduzione di Andrea Buzzi 260 $aMilano :$bLeonardo,$c1991 300 $a472 p., [8] c. di tav. :$bill. ;$c24 cm 600 14$aFoucault, Michel$xBiografie 700 1 $aBuzzi, Andrea 912 $a991004379436807536 996 $aMichel Foucault : (1926-1984)$94373873 997 $aUNISALENTO