LEADER 05338nam 2200685 450 001 9910137229203321 005 20200520144314.0 010 $a1-118-97872-2 010 $a1-118-97873-0 035 $a(CKB)3710000000514515 035 $a(EBL)4093368 035 $a(SSID)ssj0001586905 035 $a(PQKBManifestationID)16270180 035 $a(PQKBTitleCode)TC0001586905 035 $a(PQKBWorkID)14869715 035 $a(PQKB)10353620 035 $a(MiAaPQ)EBC4093368 035 $a(Au-PeEL)EBL4093368 035 $a(CaPaEBR)ebr11119461 035 $a(CaONFJC)MIL853621 035 $a(OCoLC)929851598 035 $a(PPN)197664717 035 $a(EXLCZ)993710000000514515 100 $a20151209h20162016 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 00$aAuroral dynamics and space weather /$fYongliang Zhang, Larry J. Paxton, editors ; contributors, Roger A. Anderson [and fifty-eight others] 210 1$aWashington, District of Columbia ;$aHoboken, New Jersey :$cAmerican Geophysical Union :$cWiley,$d2016. 210 4$d©2016 215 $a1 online resource (610 p.) 225 1 $aGeophysical Monograph Series ;$v215 300 $a"This work is a co-publication between the American Geophysical Union and John Wiley and Sons, Inc." 311 $a1-118-97871-4 311 $a1-118-97870-6 320 $aIncludes bibliographical references at the end of each chapters and index. 327 $aTitle Page; Table of Contents; CONTRIBUTORS; PREFACE; ACKNOWLEDGMENTS; Part I: Aurora Types and Dynamics; 1 Investigations of the Many Distinct Types of Auroras; 1.1. OVERVIEW; 1.2. DIFFUSE AURORA; 1.3. DISCRETE AURORA; 1.4. DYNAMIC AURORA AND SMALL-SCALE AURORAL STRUCTURES; REFERENCES; 2 Quasiperiodic Aurora: Outstanding Problems and Recent Results; 2.1. INTRODUCTION; 2.2. FLICKERING AURORA; 2.3. PULSATING AURORA; 2.4. CONCLUDING REMARKS; ACKNOWLEDGMENTS; REFERENCES; 3 Inverted-V Auroral Arcs and Alfve?n Waves; 3.1. INTRODUCTION; 3.2. OBSERVATIONS AND INTERPRETATION; 3.3. CONCLUSION 327 $aACKNOWLEDGMENTSREFERENCES; 4 Auroral Arcs and Ion Outflow; 4.1. INTRODUCTION; 4.2. ACCELERATION MECHANISMS; 4.3. OBSERVATIONS: SPATIAL DISTRIBUTION AND RELATIONSHIP WITH AURORAL ARC MORPHOLOGY; 4.4. IMPACT ON IONOSPHERIC AND MAGNETOSPHERIC DYNAMICS; 4.5. CONCLUSION; ACKNOWLEDGMENT; REFERENCES; 5 Isolated Proton Auroras and Pc1/EMIC Waves at Subauroral Latitudes; 5.1. INTRODUCTION; 5.2. OBSERVATION SITE AND INSTRUMENTATION; 5.3. EVENT DETECTION METHODS; 5.4. STATISTICAL RESULTS; 5.5. SUMMARY AND DISCUSSION; ACKNOWLEDGMENTS; REFERENCES 327 $a6 Dynamics of the Dayside Aurora as Viewed from the South Pole6.1. INTRODUCTION; 6.2. INSTRUMENTATION; 6.3. RESULTS; 6.4. DISCUSSION; 6.5. CONCLUSIONS; ACKNOWLEDGMENTS; REFERENCES; 7 Structures in Polar Rain Auroras; 7.1. INTRODUCTION; 7.2. OBSERVATIONS OF POLAR RAIN AURORA; 7.3. STATISTICAL STUDY OF POLAR RAIN ELECTRON STRUCTURES; 7.4. NIGHTSIDE POLAR RAIN GAP AND ENERGY DISPERSION; 7.5. SUMMARY; ACKNOWLEDGMENTS; REFERENCES; 8 Dynamics Related to Plasmasheet Flow Bursts as Revealed from the Aurora; 8.1. INTRODUCTION; 8.2. ASSOCIATIONS BETWEEN FLOW BURSTS AND AURORA STREAMERS 327 $a10.2. RECENT RESULTS10.3. SUMMARY; ACKNOWLEDGMENTS; REFERENCES; 11 Interhemispheric Symmetries and Asymmetries of Aurora from Ground-Based Conjugate Observations; 11.1. INTRODUCTION; 11.2. OBSERVATION; 11.3. SUMMARY AND DISCUSSION; ACKNOWLEDGMENT; REFERENCES; Part III: Substorm Aurora; 12 Magnetospheric Substorm Onset by Current Disruption Processes; 12.1. INTRODUCTION; 12.2. OBSERVATIONS OF THE SUBSTORM CURRENT SYSTEM; 12.3. THE CURRENT DISRUPTION MODEL FOR THE SUBSTORM CURRENT SYSTEM; 12.4. OBSERVATIONS PERTAINING TO SUBSTORM CURRENT SYSTEM 327 $a12.5. SOME DISTINGUISHING FEATURES BETWEEN THE TWO PREVAILING SUBSTORM MODELS 330 3 $aThe aurora is the most visible manifestation of the connection of the Earth to the space environment and has inspired awe, curiosity, and scientific inquiry for centuries. Recent advances in observing techniques and modeling and theoretical work have revealed new auroral phenomena, provided a better understanding of auroral dynamics, and have led to an enhanced capability for auroral forecasts. This monograph features discussions of: *New auroral phenomena due to the ring current ion and polar rain electron precipitation *Various auroral forms and hemispheric asymmetry *Auroral model development and MHD simulations *Application of the auroral observations for radio absorption and scintillation *Aurora nowcast and forecast for space weather operations. Auroral Dynamics and Space Weather is a valuable contribution for scientists, researchers, space weather operators, and students of Earth's space environment. 410 0$aGeophysical monograph series ;$v215. 606 $aAuroras 606 $aSpace environment 615 0$aAuroras. 615 0$aSpace environment. 676 $a538.768 702 $aZhang$b Yongliang 702 $aPaxton$b Larry J. 702 $aAnderson$b Roger A. 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910137229203321 996 $aAuroral dynamics and space weather$92155280 997 $aUNINA LEADER 03756nam 2200673Ia 450 001 9910782360803321 005 20200520144314.0 010 $a1-281-91343-X 010 $a9786611913434 010 $a1-4020-8491-9 024 7 $a10.1007/978-1-4020-8491-1 035 $a(CKB)1000000000546860 035 $a(EBL)418083 035 $a(OCoLC)311507109 035 $a(SSID)ssj0000217518 035 $a(PQKBManifestationID)11228295 035 $a(PQKBTitleCode)TC0000217518 035 $a(PQKBWorkID)10211590 035 $a(PQKB)10801318 035 $a(DE-He213)978-1-4020-8491-1 035 $a(Au-PeEL)EBL418083 035 $a(CaPaEBR)ebr10266902 035 $a(CaONFJC)MIL1101486 035 $a(Au-PeEL)EBL5292441 035 $a(CaONFJC)MIL191343 035 $a(PPN)132860570 035 $a(MiAaPQ)EBC418083 035 $a(EXLCZ)991000000000546860 100 $a20080402d2008 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 14$aThe Painleve? handbook$b[electronic resource] /$fRobert Conte, Micheline Musette 205 $a1st ed. 2008. 210 $aDordrecht $cSpringer$dc2008 215 $a1 online resource (273 p.) 300 $aDescription based upon print version of record. 311 $a94-007-9627-7 311 $a1-4020-8490-0 320 $aIncludes bibliographical references (p. 234-252) and index. 327 $aIntroduction; Singularity Analysis: Painleve? Test; Integrating Ordinary Differential Equations; Partial Differential Equations: Paieleve? Test; From the Test to Explicit Solutions of PDEs; Integration of Hamiltonian Systems; Discrete Nonlinear Equations; FAQ (Frequently Asked Questions) 330 $aNonlinear differential or difference equations are encountered not only in mathematics, but also in many areas of physics (evolution equations, propagation of a signal in an optical fiber), chemistry (reaction-diffusion systems), and biology (competition of species). This book introduces the reader to methods allowing one to build explicit solutions to these equations. A prerequisite task is to investigate whether the chances of success are high or low, and this can be achieved without any a priori knowledge of the solutions, with a powerful algorithm presented in detail called the Painlevé test. If the equation under study passes the Painlevé test, the equation is presumed integrable. If on the contrary the test fails, the system is nonintegrable or even chaotic, but it may still be possible to find solutions. The examples chosen to illustrate these methods are mostly taken from physics. These include on the integrable side the nonlinear Schrödinger equation (continuous and discrete), the Korteweg-de Vries equation, the Hénon-Heiles Hamiltonians, on the nonintegrable side the complex Ginzburg-Landau equation (encountered in optical fibers, turbulence, etc), the Kuramoto-Sivashinsky equation (phase turbulence), the Kolmogorov-Petrovski-Piskunov equation (KPP, a reaction-diffusion model), the Lorenz model of atmospheric circulation and the Bianchi IX cosmological model. Written at a graduate level, the book contains tutorial text as well as detailed examples and the state of the art on some current research. 606 $aPainleve? equations 606 $aMathematical physics 615 0$aPainleve? equations. 615 0$aMathematical physics. 676 $a515.352 676 $a518/.6 700 $aConte$b Robert$f1943-$0891610 701 $aMusette$b Micheline$0731201 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910782360803321 996 $aThe Painleve? handbook$93768140 997 $aUNINA