000 03821nam a22005415i 4500
001 978-3-540-71570-2
003 DE-He213
005 20190213151334.0
007 cr nn 008mamaa
008 100301s2007 gw | s |||| 0|eng d
020 _a9783540715702
_9978-3-540-71570-2
024 7 _a10.1007/978-3-540-71570-2
_2doi
050 4 _aQB1-991
050 4 _aQB460-466
050 4 _aQB980-991
072 7 _aPGC
_2bicssc
072 7 _aSCI004000
_2bisacsh
072 7 _aPGC
_2thema
082 0 4 _a520
_223
245 1 4 _aThe High Energy Solar Corona: Waves, Eruptions, Particles
_h[electronic resource] /
_cedited by Karl-Ludwig Klein, Alexander L. MacKinnon.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c2007.
300 _aX, 284 p.
_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 ;
_v725
505 0 _aIntroduction: The High-energy Corona – Waves, Eruptions, Particles -- Introduction: The High-energy Corona – Waves, Eruptions, Particles -- Particle Acceleration During Flares -- Magnetic Complexity, Fragmentation, Particle Acceleration and Radio Emission from the Sun -- Review of Selected RHESSI Solar Results -- RHESSI Results – Time for a Rethink? -- Small Scale Energy Release and the Acceleration and Transport of Energetic Particles -- Large-scale Disturbances -- Large-scale Waves and Shocks in the Solar Corona -- Energetic Particles Related with Coronal and Interplanetary Shocks -- Particle Acceleration at the Earth’s Bow Shock -- On the Existence of Non-maxwellian Velocity Distribution Functions in the Corona and their Consequences for the Solar Wind Acceleration -- Recent Research: Large-scale Disturbances, their Origin and Consequences -- Plasma of the Solar Corona -- Quasi-periodic Pulsations as a Diagnostic Tool for Coronal Plasma Parameters -- Pulsating Solar Radio Emission.
520 _aAn outgrowth of a workshop held by the Community of European Solar Radio Astronomers (CESRA), this volume collects reviews on current research and perspectives on the variable solar corona: high-energy particles, large-scale disturbances such as mass ejections and waves, and radio diagnostics of the coronal plasma. Multiwavelength observations of the Sun with radio instruments and recent space missions are drawn on extensively, as well as input from neighbouring fields e.g. solar wind, Earth's bow shock. Recent developments are discussed alongside key developments in this rapidly evolving field.
650 0 _aAstronomy.
650 0 _aPhysical geography.
650 1 4 _aAstronomy, Astrophysics and Cosmology.
_0http://scigraph.springernature.com/things/product-market-codes/P22006
650 2 4 _aAtoms and Molecules in Strong Fields, Laser Matter Interaction.
_0http://scigraph.springernature.com/things/product-market-codes/P24025
650 2 4 _aPlasma Physics.
_0http://scigraph.springernature.com/things/product-market-codes/P24040
650 2 4 _aGeophysics/Geodesy.
_0http://scigraph.springernature.com/things/product-market-codes/G18009
700 1 _aKlein, Karl-Ludwig.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
700 1 _aMacKinnon, Alexander L.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9783642090769
776 0 8 _iPrinted edition:
_z9783540836803
776 0 8 _iPrinted edition:
_z9783540715696
830 0 _aLecture Notes in Physics,
_x0075-8450 ;
_v725
856 4 0 _uhttps://doi.org/10.1007/978-3-540-71570-2
912 _aZDB-2-PHA
912 _aZDB-2-LNP
999 _c10328
_d10328