LEADER 05086nam 2200625Ia 450 001 9910830631503321 005 20230803031002.0 010 $a3-527-65207-8 010 $a3-527-65205-1 010 $a3-527-65208-6 035 $a(CKB)2670000000403757 035 $a(EBL)1329760 035 $a(OCoLC)854977486 035 $a(SSID)ssj0001034853 035 $a(PQKBManifestationID)11592307 035 $a(PQKBTitleCode)TC0001034853 035 $a(PQKBWorkID)11017395 035 $a(PQKB)10307140 035 $a(MiAaPQ)EBC1329760 035 $a(MiAaPQ)EBC4044356 035 $a(EXLCZ)992670000000403757 100 $a20121015d2013 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aMagnetoseismology$b[electronic resource] $eground-based remote sensing of Earth's magnetosphere /$fFrederick W. Menk and Colin L. Waters 210 $aWeinheim $cWiley-VCH$dc2013 215 $a1 online resource (281 p.) 300 $aDescription based upon print version of record. 311 $a1-299-75964-5 311 $a3-527-41027-9 320 $aIncludes bibliographical references and index. 327 $aMagnetoseismology: Ground-based remote sensing of the Earth's magnetosphere; Contents; Preface; Color Plates; 1 Introduction; 1.1 Purpose of This Book; 1.2 The Solar Wind; 1.3 Fluctuations in the Solar Wind; 1.4 Early Observations of Geomagnetic Variations; 1.5 Properties of Geomagnetic Variations; 2 The Magnetosphere and Ionosphere; 2.1 The Geomagnetic Field; 2.2 Structure of Earth's Magnetosphere; 2.3 Magnetospheric Current Systems; 2.3.1 Magnetopause Current; 2.3.2 Tail Current and Reconnection; 2.3.3 Ring Current; 2.3.4 Field-Aligned Currents; 2.3.5 Ionospheric Currents 327 $a2.4 The Radiation Belts2.5 The Inner Magnetosphere; 2.6 Formation and Properties of the Ionosphere; 2.7 Geomagnetic Disturbances; 2.8 Space Weather Effects; 3 ULF Plasma Waves in the Magnetosphere; 3.1 Basic Properties of a Plasma; 3.2 Particle Motions; 3.2.1 Motions of Isolated Charged Particles; 3.2.2 First Adiabatic Invariant; 3.2.3 Second Adiabatic Invariant; 3.2.4 Third Adiabatic Invariant; 3.3 Low-Frequency Magnetized Plasma Waves; 3.3.1 Equations of Linear MHD; 3.3.2 The Wave Equation; 3.4 The Shear Alfv en Mode in a Dipole Magnetic Field; 3.4.1 Toroidal Oscillation of Field Lines 327 $a3.5 MHD Wave Mode Coupling in One Dimension3.6 An Alternative Derivation of the Plasma Wave Equation, from Electromagnetism; 4 Sources of ULF Waves; 4.1 Introduction; 4.2 Exogenic Sources; 4.3 Boundary Instabilities; 4.4 Field Line Resonances; 4.5 Cavity and Waveguide Modes; 4.6 Spatially Localized Waves; 4.7 Ion Cyclotron Waves; 5 Techniques for Detecting Field Line Resonances; 5.1 Introduction; 5.2 Variation in Spectral Power with Latitude; 5.3 Variation of Phase with Latitude; 5.4 Wave Polarization Properties; 5.5 Spectral Power Difference and Division; 5.6 Single Station H/D 327 $a5.7 Cross-Phase from Latitudinally Separated Sensors5.8 Using ULF Wave Polarization Properties; 5.9 Automated Detection Algorithms; 6 Ground-Based Remote Sensing of the Magnetosphere; 6.1 Estimating Plasma Mass Density; 6.2 Travel Time Method of Tamao; 6.3 Determining Electron Density; 6.4 Verification of Ground-Based Mass Density Measurements; 6.5 Determining Ion Concentrations; 6.6 Field-Aligned Plasma Density; 6.7 Plasma Density at Low Latitudes; 6.8 Plasma Density at High Latitudes; 7 Space Weather Applications; 7.1 Magnetospheric Structure and Density; 7.2 Plasmapause Dynamics 327 $a7.3 Density Notches, Plumes, and Related Features7.4 Refilling of the Plasmasphere; 7.5 Longitudinal Variation in Density; 7.6 Solar Cycle Variations in Density; 7.7 Determining the Open/Closed Field Line Boundary; 7.8 Determining the Magnetospheric Topology at High Latitudes; 7.9 Wave-Particle Interactions; 7.10 Radial Motions of Flux Tubes; 8 ULF Waves in the Ionosphere; 8.1 Introduction; 8.2 Electrostatic and Inductive Ionospheres; 8.3 ULF Wave Solution for a Thin Sheet Ionosphere; 8.4 ULF Wave Solution for a Realistic Ionosphere; 8.5 FLRs and the Ionosphere 327 $a8.6 Remote Sensing ULF Electric Fields in Space 330 $aThis book provides a comprehensive account of magnetoseismology - the tool to monitor space weather. Written by researcher on the forefront of this field, it conveys the physics behind the phenomena and the methods to detect and investigate them, the relevance to communication, power supply and many other critical systems. In addition, it provides computational codes for analysis and evaluation. 606 $aMagnetosphere 606 $aMagnetospheric physics 615 0$aMagnetosphere. 615 0$aMagnetospheric physics. 676 $a538.766 700 $aMenk$b Frederick W$01612548 701 $aWaters$b Colin L$01612549 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910830631503321 996 $aMagnetoseismology$93941405 997 $aUNINA