05594nam 2200721 450 991013230220332120200520144314.01-118-84229-41-118-84232-41-118-84237-5(CKB)3710000000321368(EBL)1895649(SSID)ssj0001434923(PQKBManifestationID)11782830(PQKBTitleCode)TC0001434923(PQKBWorkID)11433572(PQKB)10859219(Au-PeEL)EBL1895649(CaPaEBR)ebr11005789(CaONFJC)MIL769965(OCoLC)898770166(MiAaPQ)EBC1895649(PPN)191637807(EXLCZ)99371000000032136820150131h20152015 uy| 0engur|n|---|||||txtccrMagnetotails in the solar system /Andreas Keiling, Caitríona M. Jackman, Peter A. Delamere, editorsHoboken, New Jersey :Wiley,[2015]©20151 online resource (420 p.)Geophysical monograph ;207"This work is a co-publication between the American Geophysical Union and John Wiley and Sons, Inc.1-118-84234-0 Includes bibliographical references and index.Title 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; ReferencesChapter 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 Convection4.5. 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; ReferencesChapter 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 WakeAcknowledgmentsReferences; 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. Introduction12.2. Terrestrial Tail Formation: Solar Wind Reconnection Dominant 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 magnetospGeophysical monograph series ;no. 207.MagnetospherePlanetsAtmospheresSolar systemMagnetosphere.PlanetsAtmospheres.538.76609992Keiling AndreasJackman Caitríona M.Delamere Peter A.American Geophysical Union,MiAaPQMiAaPQMiAaPQBOOK9910132302203321Magnetotails in the solar system2040552UNINA