Quasi linear transport equation systems shocks formation

Studies of resonant flow instabilities in MHD involve the generalisation of stability theory when resonance occurs in a steady plasma. studying the processes of randomВ energy deposition in magnetic flux tubes.proposing a unified modelВ for explosive events and blinkers.deriving the observational signaturesВ of micro-scale reconnection.Studies of nano-scale reconnection MHD heating under solar atmospheric conditions. developing the tools of global coronal seismology.sunspots, magnetic canopy, fibrils, coronal loops and magnetosphere) making successful applicationsВ of resonant MHD wave theory (e.g.proof of the validity of the universal characterВ of the jump conditions in dissipative MHD and in dilute plasmas.These universal connection formulae play a crucial role, similar to the Rankine-Hugoniot relations of nonlinear gas dynamics obtaining jump conditionsВ to connect solutions across a resonant layer.derivation of the generalised governing equationВ for resonant slow MHD waves in isotropic and anisotropic steady plasmas.Studies of linear and nonlinear resonant MHD wave heating under solar atmospheric conditions. Prepared a 'Handbook for Teachers in Astronomy', 1987, (approx.'The Beginning of Greek Astronomy' ( 2nd prizeВ at bi-annual CHRS, 1987, Eger, Hungary).for Hungarian Research Students (History), 1987, PГ©cs, Hungary) History of the ancient Far-East and Greece: 'Save of Mohenjo-daro' ( 1st prize with Highest DistinctionВ at bi-annual Conf.Prepared a 'Collection of Hungarian-Sanskrit Terminus Technicus in Astronomy' for historical studies (1988).of Astronomy, EГ¶tvГ¶s U., Budapest, Hungary 09/1998-10/2001 Lecturer, Department of Applied Mathematics, The University of Sheffield.11/2001 Reader, Department of Applied Mathematics, The University of Sheffield.09/2003 Professor, Department of Applied Mathematics, The University of Sheffield.UKSP: Chair to UK Solar Physics from 2002.

UKSP: Secretary to UK Solar Physics till 12/2001.MTA-OTT: Society of Antiquity History, Hungarian Academy of Sciences.MTA: Assembly Member of Hungarian Academy of Sciences and Arts.AAS: American Astronomical Society (USA).Membership of Learned Societies/Professional Bodies 1988 M.Sc.В both in PhysicsВ and Astronomy, EГ¶tvГ¶s U., Budapest, Hungary.1996 PhD (Applied Maths.В with Summa cum laude, K.U.Leuven, Belgium.The Candidatus of Science degree is one higher than the PhD 1997 CSc(Physics)В (Candidatus of Science) with Summa cum laude, Hungarian Academy of Sciences, Budapest, Hungary.Qualifications Education and qualification after school Computational Magnetohydrodynamics (CMHD).My current projects (find out more in Research interests) in SPARG include: I became Head of the Solar Physics & Upper-Atmosphere Research Group (SPARG) in the Department of Applied Mathematics in 2004. magnetohydrodynamics, computational fluid dynamics, kinetic theory) has direct applications in the new and rapidly emerging discipline of helioseismology and space weather. My interdisciplinary research (including e.g. Understanding the subtleties of plasma confinement at high temperatures is also strongly linked to modern fusion physics. Particular attention is paid to the solar influence on the magnetosphere and space weather. The aim of my research is to address these questions through theoretical (both numerical and exact analytical methods) and observational studies (joint ground-based and satellite missions). The heating processes that generate and sustain the observed high temperature of the solar and stellar atmospheres have so far defied a quantitative understanding despite the multitude of efforts spanning over half a century. My main research interests lie in the general field of space plasma physics. Support for refugee students and scholars.Conferences, events, visitor accommodation and weddings.

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Quasi linear transport equation systems shocks formation