LEADER 01416nam0 2200361 450 001 000022673 005 20090203170249.0 100 $a20081022d1930----km-y0itaa50------ba 101 0 $afre 102 $aFR 200 1 $a<> chose judiciaire$fLouise Roubaud$gpréface de Bernard Grasset 205 $a12. ed 210 $aParis$c<> Grasset$dc1930 215 $aXVIII, 321 p.$d19 cm. 300 $aIn cop. e in testa al front.firma autografa: Sergio de Pilato, aprile '930, VIII 607 $aFrancia$xOrdinamento giudiziario 676 $a349.44$v(21. ed.)$9Diritto di singoli Stati e Nazioni (Diritto interno). Francia e Monaco 676 $a306.250944$v(21. ed.)$9Istituzioni giudiziarie. Francia 700 1$aRoubaud,$bLouis$0443938 801 0$aIT$bUniversità della Basilicata - B.I.A.$gRICA$2unimarc 912 $a000022673 996 $aChose judiciaire$987465 997 $aUNIBAS BAS $aLETTERE CAT $aSTD069$b01$c20081022$lBAS01$h1533 CAT $aSTD069$b01$c20081022$lBAS01$h1538 CAT $aSTD069$b01$c20081118$lBAS01$h1439 CAT $aTTM$b30$c20090203$lBAS01$h1650 CAT $aTTM$b30$c20090203$lBAS01$h1654 CAT $aTTM$b30$c20090203$lBAS01$h1701 CAT $aTTM$b30$c20090203$lBAS01$h1702 FMT Z30 -1$lBAS01$LBAS01$mBOOK$1BASA1$APolo Storico-Umanistico$2FDEP2$BFondo De Pilato Biscione$3FD/107471$6107471$5L107471$820090128$f52$FRari LEADER 04690nam 22006135 450 001 9910869183603321 005 20240629125227.0 010 $a9783031581779 024 7 $a10.1007/978-3-031-58177-9 035 $a(CKB)32609882900041 035 $a(MiAaPQ)EBC31507302 035 $a(Au-PeEL)EBL31507302 035 $a(DE-He213)978-3-031-58177-9 035 $a(EXLCZ)9932609882900041 100 $a20240629d2024 u| 0 101 0 $aeng 135 $aur||||||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aEruptions on the Sun /$fby Boris Filippov 205 $a1st ed. 2024. 210 1$aCham :$cSpringer Nature Switzerland :$cImprint: Springer,$d2024. 215 $a1 online resource (400 pages) 225 1 $aAstrophysics and Space Science Library,$x2214-7985 ;$v471 311 08$a9783031581762 320 $aIncludes bibliographical references and index. 327 $aIntroduction -- General Characteristics of the Sun -- Magnetic Fields on the Sun -- Equilibrium Plasma Structures in the Solar Atmosphere -- Intimate relationship between plasma structures and magnetic fields in the solar atmosphere -- Peculiarities of the Filament Visual Interaction on the Solar Disk -- Eruption of Prominences -- Causes of prominence eruptions -- Solar Jets -- Solar Flares -- Coronal Mass Ejections -- Solar Wind and Space Weather. 330 $aThis book is devoted to eruptive phenomena on the Sun, the most dangerous sources of space weather disturbances. It discusses the latest achievements in this field, described in the scientific literature and obtained by the author himself. The initial chapters of the book give a brief description of the role of the Sun in the life and history of mankind, a general description of the solar interior and the atmosphere of the Sun, the causes and drivers of solar activity and its impact on the Earth's environment and human life. The book provides a detailed description of eruptive phenomena on the Sun, a review of observations of solar activity and theoretical ideas about the mechanisms and causes of a sudden release of energy in the solar atmosphere. Much attention is paid to the solar magnetic fields, their characteristic features and measured values in the photosphere, the observed manifestations in the chromosphere and corona, and methods for extrapolating photospheric data to the upper layers of the solar atmosphere. It is assumed that the magnetic field is the source of energy suddenly released during eruptive phenomena observed in the form of flares, prominence eruptions and coronal mass ejections (CMEs). Energy is accumulated and stored in the non-potential (associated with electric currents) part of the coronal magnetic field (free magnetic energy). This part of the field is the most variable and can provide energy for fast eruptive processes. CMEs, propagating through the interplanetary medium, significantly perturb it and cause the strongest geomagnetic storms when they affect the Earth's magnetosphere. The prediction of the arrival of the CME is the key problem of the entire space weather forecast. Thus, pre-eruptive conditions in CME source regions are of great importance. Solar prominences and filaments are considered the most likely progenitors of CMEs. Most of the book is devoted to the description and analysis of their equilibrium and stability. It is shown that there are measurable characteristics of the proximity of the prominence to the instability threshold, which can be very useful in the problem of space weather forecasting. The book contains many illustrations and links to the latest scientific articles and reviews on the topic. It will be useful to researchers in the field of astrophysics, solar physics, geophysics, as well as PhD and graduate students. 410 0$aAstrophysics and Space Science Library,$x2214-7985 ;$v471 606 $aSun 606 $aAstrophysics 606 $aAstronomy$xObservations 606 $aPlasma astrophysics 606 $aSolar Physics 606 $aAstrophysics 606 $aAstronomy, Observations and Techniques 606 $aAstrophysical Plasma 615 0$aSun. 615 0$aAstrophysics. 615 0$aAstronomy$xObservations. 615 0$aPlasma astrophysics. 615 14$aSolar Physics. 615 24$aAstrophysics. 615 24$aAstronomy, Observations and Techniques. 615 24$aAstrophysical Plasma. 676 $a551.5 700 $aFilippov$b Boris$0610973 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 912 $a9910869183603321 996 $aEruptions on the Sun$94170597 997 $aUNINA