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020 _a9783540691242
_9978-3-540-69124-2
024 7 _a10.1007/BFb0105667
_2doi
050 4 _aQB4
072 7 _aPG
_2bicssc
072 7 _aSCI004000
_2bisacsh
072 7 _aPG
_2thema
082 0 4 _a520
_223
245 1 0 _aSolar and Heliospheric Plasma Physics
_h[electronic resource] :
_bProceedings of the 8th European Meeting on Solar Physics Held at Halkidiki, Greece, 13–18 May 1996 /
_cedited by George M. Simnett, Constantine E. Alissandrakis, Loukas Vlahos.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c1997.
300 _aVIII, 280 p. 107 illus., 1 illus. in color.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aLecture Notes in Physics,
_x0075-8450 ;
_v489
505 0 _aThe 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.
520 _aThis 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.
650 0 _aAstrophysics.
650 0 _aQuantum theory.
650 1 4 _aAstronomy, Observations and Techniques.
_0http://scigraph.springernature.com/things/product-market-codes/P22014
650 2 4 _aAstrophysics and Astroparticles.
_0http://scigraph.springernature.com/things/product-market-codes/P22022
650 2 4 _aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
_0http://scigraph.springernature.com/things/product-market-codes/P22030
650 2 4 _aAtomic, Molecular, Optical and Plasma Physics.
_0http://scigraph.springernature.com/things/product-market-codes/P24009
650 2 4 _aElementary Particles, Quantum Field Theory.
_0http://scigraph.springernature.com/things/product-market-codes/P23029
700 1 _aSimnett, George M.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
700 1 _aAlissandrakis, Constantine E.
_eeditor.
_4edt
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700 1 _aVlahos, Loukas.
_eeditor.
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710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9783662141441
776 0 8 _iPrinted edition:
_z9783662141434
776 0 8 _iPrinted edition:
_z9783540630722
830 0 _aLecture Notes in Physics,
_x0075-8450 ;
_v489
856 4 0 _uhttps://doi.org/10.1007/BFb0105667
912 _aZDB-2-PHA
912 _aZDB-2-LNP
912 _aZDB-2-BAE
999 _c10102
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