04976nam 22007935 450 99646671640331620200704010405.03-540-69124-310.1007/BFb0105667(CKB)1000000000778107(SSID)ssj0000326744(PQKBManifestationID)12118525(PQKBTitleCode)TC0000326744(PQKBWorkID)10297350(PQKB)10371966(DE-He213)978-3-540-69124-2(PPN)155190504(EXLCZ)99100000000077810720121227d1997 u| 0engurnn|008mamaatxtccrSolar and Heliospheric Plasma Physics[electronic resource] Proceedings of the 8th European Meeting on Solar Physics Held at Halkidiki, Greece, 13–18 May 1996 /edited by George M. Simnett, Constantine E. Alissandrakis, Loukas Vlahos1st ed. 1997.Berlin, Heidelberg :Springer Berlin Heidelberg :Imprint: Springer,1997.1 online resource (VIII, 280 p. 107 illus., 1 illus. in color.) Lecture Notes in Physics,0075-8450 ;489Bibliographic Level Mode of Issuance: Monograph3-540-63072-4 The structure and dynamics of the sun from helioseismology, and the neutrino problem -- Modulation of solar and stellar activity cycles -- Dynamics of flux tubes in the solar atmosphere: Observations -- Dynamics of flux tubes in the solar atmosphere: Theory -- Observations of energetic ions during the ulysses mission -- Solar wind and interstellar medium coupling -- Flows through the magnetically structured solar atmosphere -- Chromospheric dynamics — What can be learnt from numerical simulations -- Topologically forced reconnection -- Energy release processes in active regions -- Production of flare accelerated particles at the sun -- New ground-based solar instrumentation -- Future space instrumentation for solar physics.This volume brings together theoretical ideas on the plasma physics of both hot and dense plasmas in the solar atmosphere and similar physics applied to the tenuous and cooler plasmas found in the heliosphere. It is complemented by recent observations. Helioseismology covers the solar interior and the neutrino problem. Solar and stellar activity cycles are addressed. The dynamics of magnetic flux tubes in the solar atmosphere and material flows through the chromosphere into the upper atmosphere are comprehensively reviewed. Energy release processes and the production of energetic particles are important to understanding events in the solar atmosphere and to the dynamics of the tenuous heliosphere. A glimpse of the future is offered by concluding chapters on new ground-based and space instrumentation.Lecture Notes in Physics,0075-8450 ;489Observations, AstronomicalAstronomy—ObservationsAstrophysicsSpace sciencesAtomsPhysicsElementary particles (Physics)Quantum field theoryAstronomy, Observations and Techniqueshttps://scigraph.springernature.com/ontologies/product-market-codes/P22014Astrophysics and Astroparticleshttps://scigraph.springernature.com/ontologies/product-market-codes/P22022Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)https://scigraph.springernature.com/ontologies/product-market-codes/P22030Atomic, Molecular, Optical and Plasma Physicshttps://scigraph.springernature.com/ontologies/product-market-codes/P24009Elementary Particles, Quantum Field Theoryhttps://scigraph.springernature.com/ontologies/product-market-codes/P23029Observations, Astronomical.Astronomy—Observations.Astrophysics.Space sciences.Atoms.Physics.Elementary particles (Physics).Quantum field theory.Astronomy, Observations and Techniques.Astrophysics and Astroparticles.Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).Atomic, Molecular, Optical and Plasma Physics.Elementary Particles, Quantum Field Theory.523.7Simnett George Medthttp://id.loc.gov/vocabulary/relators/edtAlissandrakis Constantine Eedthttp://id.loc.gov/vocabulary/relators/edtVlahos Loukasedthttp://id.loc.gov/vocabulary/relators/edtEuropean Meeting on Solar PhysicsBOOK996466716403316Solar and Heliospheric Plasma Physics2510524UNISA