LEADER 03350nam 2200589 450 001 9910146553403321 005 20220514081314.0 010 $a3-540-71570-3 024 7 $a10.1007/978-3-540-71570-2 035 $a(CKB)1000000000492204 035 $a(SSID)ssj0000318094 035 $a(PQKBManifestationID)11923573 035 $a(PQKBTitleCode)TC0000318094 035 $a(PQKBWorkID)10308781 035 $a(PQKB)11450550 035 $a(DE-He213)978-3-540-71570-2 035 $a(MiAaPQ)EBC3061872 035 $a(MiAaPQ)EBC6711191 035 $a(Au-PeEL)EBL6711191 035 $a(OCoLC)1273972234 035 $a(PPN)12372709X 035 $a(EXLCZ)991000000000492204 100 $a20220514d2007 uy 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 04$aThe high energy solar corona $ewaves, eruptions, particles /$fK.-L. Klein, A. L. MacKinnon (editors) 205 $a1st ed. 2007. 210 1$aBerlin ;$aHeidelberg :$cSpringer-Verlag,$d[2007] 210 4$dİ2007 215 $a1 online resource (X, 284 p.) 225 1 $aLecture notes in physics ;$v725 300 $aBibliographic Level Mode of Issuance: Monograph 311 $a3-540-71569-X 327 $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. 330 $aAn outgrowth of a workshop held by the Community of European Solar Radio Astronomers (CESRA), this volume collects reviews on current research and perspectives on the variable solar corona: high-energy particles, large-scale disturbances such as mass ejections and waves, and radio diagnostics of the coronal plasma. Multiwavelength observations of the Sun with radio instruments and recent space missions are drawn on extensively, as well as input from neighbouring fields e.g. solar wind, Earth's bow shock. Recent developments are discussed alongside key developments in this rapidly evolving field. 410 0$aLecture notes in physics ;$v725. 606 $aSolar energetic particles 607 $aSun$xCorona 615 0$aSolar energetic particles. 676 $a523.75 702 $aKlein$b L$g(Ludwig),$f1954- 702 $aMacKinnon$b A. L$g(Alexander L.), 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910146553403321 996 $aThe high energy solar corona$92843011 997 $aUNINA