LEADER 05594nam 2200721 450 001 9910807442003321 005 20200520144314.0 010 $a1-118-84229-4 010 $a1-118-84232-4 010 $a1-118-84237-5 035 $a(CKB)3710000000321368 035 $a(EBL)1895649 035 $a(SSID)ssj0001434923 035 $a(PQKBManifestationID)11782830 035 $a(PQKBTitleCode)TC0001434923 035 $a(PQKBWorkID)11433572 035 $a(PQKB)10859219 035 $a(Au-PeEL)EBL1895649 035 $a(CaPaEBR)ebr11005789 035 $a(CaONFJC)MIL769965 035 $a(OCoLC)898770166 035 $a(MiAaPQ)EBC1895649 035 $a(PPN)191637807 035 $a(EXLCZ)993710000000321368 100 $a20150131h20152015 uy| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 00$aMagnetotails in the solar system /$fAndreas Keiling, Caitri?ona M. Jackman, Peter A. Delamere, editors 210 1$aHoboken, New Jersey :$cWiley,$d[2015] 210 4$dİ2015 215 $a1 online resource (420 p.) 225 1 $aGeophysical monograph ;$v207 300 $a"This work is a co-publication between the American Geophysical Union and John Wiley and Sons, Inc. 311 $a1-118-84234-0 320 $aIncludes bibliographical references and index. 327 $aTitle Page; Copyright Page; Contents; Contributors; Preface; Section I: Introduction; Chapter 1 Magnetotail: Unsolved Fundamental Problem of Magnetospheric Physics; 1.1. Introduction; 1.2. Essential Properties; 1.3. Global Stress Balance Problem; 1.4. What Maintains a Magnetotail?; 1.5. Conclusion; APPENDIX: Some Questions about Internal Pressure; Acknowledgments; References; Section II: Tutorials; Chapter 2 Mercury's Magnetotail; 2.1. Introduction; 2.2. Planetary Magnetic Field; 2.3. Magnetosphere; 2.4. External Driving; 2.5. Tail Dynamics; 2.6. Summary; References 327 $aChapter 3 Magnetotails of Mars and Venus3.1. Introduction; 3.2. General Features of Magnetotails on Mars and Venus; 3.3. Ion Acceleration; 3.4. Bursty Flows; 3.5. Reconnection in Induced Tails; 3.6. Pressure Balance and Asymmetry of Plasma Sheet; 3.7. Ion Escape through Tails; 3.8. Induced Magnetic Tails for Flow Aligned IMF; 3.9. Effect of Crustal Fields on Near-Mars Tail; 3.10. Conclusions; Acknowledgments; References; Chapter 4 Earth's Magnetotail; 4.1. Introduction; 4.2. Dynamic Magnetotail; 4.3. Magnetospheric Substorm; 4.4. Steady Magnetospheric Convection 327 $a4.5. Sawtooth Injection Events4.6. Pseudo Breakups; 4.7. Poleward Boundary Intensifications; 4.8. Questions Related to Dynamics of Magnetotail; Acknowledgments; References; Chapter 5 Jupiter's Magnetotail; 5.1. Introduction; 5.2. Particle Parameters of Jupiter's Magnetotail; 5.3. Energetic Events and Magnetic Reconnection; 5.4. Summary; 5.5. Future Exploration; Acknowledgments; References; Chapter 6 Saturn's Magnetotail; 6.1. Introduction; 6.2. Large-Scale Tail Structure; 6.3. Magnetospheric Dynamics; 6.4. Remote Sensing of Tail Dynamics; 6.5. Discussion; Acknowledgments; References 327 $aChapter 7 Magnetotails of Uranus and Neptune7.1. Introduction; 7.2. Magnetospheres of Uranus and Neptune; 7.3. Magnetotail Configuration at Uranus and Neptune; 7.4. Magnetotail Dynamics; 7.5. Discussion; Acknowledgments; References; Chapter 8 Satellite Magnetotails; 8.1. Introduction; 8.2. Inert Moons; 8.3. Conducting/Mass-Loading Moons; 8.4. A Strongly Magnetized Moon: Ganymede; 8.5. Summary; Acknowledgments; References; Chapter 9 Moon's Plasma Wake; 9.1. Introduction; 9.2. Structure and Dynamics of Lunar Wake; 9.3. Simulations of Lunar Wake; 9.4. Frontiers in Study of Lunar Wake 327 $aAcknowledgmentsReferences; Chapter 10 Physics of Cometary Magnetospheres; 10.1. Introduction; 10.2. The Coma; 10.3. Mass Loading; 10.4. Mathematical Description; 10.5. Bow Shock and Cometosheath; 10.6. Cometary Magnetotails; 10.7. Model-Data Comparison; 10.8. Rosetta; Acknowledgments; References; Chapter 11 Heliotail; 11.1. Introduction; 11.2. Observations of the Heliotail; 11.3. Discussion; Acknowledgments; References; Section III: Specialized Topics; Chapter 12 Formation of Magnetotails: Fast and Slow Rotators Compared; 12.1. Introduction 327 $a12.2. Terrestrial Tail Formation: Solar Wind Reconnection Dominant 330 $a All magnetized planets in our solar system (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) interact strongly with the solar wind and possess well developed magnetotails. It is not only the strongly magnetized planets that have magnetotails. Mars and Venus have no global intrinsic magnetic field, yet they possess induced magnetotails. Comets have magnetotails that are formed by the draping of the interplanetary magnetic field. In the case of planetary satellites (moons), the magnetotail refers to the wake region behind the satellite in the flow of either the solar wind or the magnetosp 410 0$aGeophysical monograph series ;$vno. 207. 606 $aMagnetosphere 606 $aPlanets$xAtmospheres 607 $aSolar system 615 0$aMagnetosphere. 615 0$aPlanets$xAtmospheres. 676 $a538.76609992 702 $aKeiling$b Andreas 702 $aJackman$b Caitri?ona M. 702 $aDelamere$b Peter A. 712 02$aAmerican Geophysical Union, 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910807442003321 996 $aMagnetotails in the solar system$94001357 997 $aUNINA