05065nam 22008175 450 99646671560331620200706031247.03-540-36242-810.1007/3-540-36242-8(CKB)1000000000777897(SSID)ssj0000322900(PQKBManifestationID)12091392(PQKBTitleCode)TC0000322900(PQKBWorkID)10296143(PQKB)11220380(DE-He213)978-3-540-36242-5(MiAaPQ)EBC3073153(PPN)155174207(EXLCZ)99100000000077789720121227d2003 u| 0engurnn|008mamaatxtccrEnergy Conversion and Particle Acceleration in the Solar Corona[electronic resource] /edited by Karl-Ludwig Klein1st ed. 2003.Berlin, Heidelberg :Springer Berlin Heidelberg :Imprint: Springer,2003.1 online resource (X, 319 p.) Lecture Notes in Physics,0075-8450 ;612Bibliographic Level Mode of Issuance: Monograph3-540-00275-8 Includes bibliographical references at the end of each chapters and index.Energy Release and Magnetic Reconnection -- Magnetic Reconnection on the Sun and in the Earth’s Magnetosphere -- Magnetic 3-D Configurations of Energy Release in Solar Flares -- Theoretical Models of Magnetic Configurations Relevant to Energy Release -- The Energy Release Process in Solar Flares; Constraints from TRACE Observations -- Radio Diagnostics of Flare Energy Release -- Signature of Energy Release and Particle Acceleration Observed by the Nobeyama Radioheliograph -- How Well Do We Understand Magnetic Reconnection? -- Energetic Particles at and from the Sun -- What Can Be Learned About Competing Acceleration Models from Multiwavelength Observations? -- Transport of Energy from the Corona to the Chromosphere During Flares -- On the Origin of Solar Energetic Particle Events -- Acceleration and Propagation of Solar Energetic Particles -- Particle Acceleration by Magnetic Reconnection -- Particle Acceleration Processes in Cosmic Plasmas -- Aspects of Current Research -- Recent Progress in Understanding Energy Conversion and Particle Acceleration in the Solar Corona -- Solar Observations at Submillimeter Wavelengths.The conversion of energy generated in the Sun's interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from the sun, the present volume reviews the current theoretical and experimental status in the field. Paying attention to both the details and the broader picture, this book addresses both the experienced researcher as well as non-specialist researchers from related areas and postgraduate students.Lecture Notes in Physics,0075-8450 ;612Space sciencesObservations, AstronomicalAstronomy—ObservationsAstrophysicsAtomsPhysicsPlasma (Ionized gases)Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)https://scigraph.springernature.com/ontologies/product-market-codes/P22030Astronomy, Observations and Techniqueshttps://scigraph.springernature.com/ontologies/product-market-codes/P22014Astrophysics and Astroparticleshttps://scigraph.springernature.com/ontologies/product-market-codes/P22022Atoms and Molecules in Strong Fields, Laser Matter Interactionhttps://scigraph.springernature.com/ontologies/product-market-codes/P24025Plasma Physicshttps://scigraph.springernature.com/ontologies/product-market-codes/P24040SunCoronaSpace sciences.Observations, Astronomical.Astronomy—Observations.Astrophysics.Atoms.Physics.Plasma (Ionized gases).Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).Astronomy, Observations and Techniques.Astrophysics and Astroparticles.Atoms and Molecules in Strong Fields, Laser Matter Interaction.Plasma Physics.523.7/5Klein Karl-Ludwigedthttp://id.loc.gov/vocabulary/relators/edtCESRA Workshop and Euroconference Energy Conversion and Particle Acceleration in the Solar Corona(2001 :Schloss Ringberg)MiAaPQMiAaPQMiAaPQBOOK996466715603316Energy conversion and particle acceleration in the solar corona376919UNISA