LEADER 01167nam0 22002773i 450 001 SUN0060929 005 20070904120000.0 010 $a88-492-0299-7 100 $a20070904d2002 |0itac50 ba 101 $aita 102 $aIT 105 $a|||| ||||| 200 1 $aˆL'‰ambiente urbano di Catania nel '900$ele architetture degli anni '20$fMariateresa Galizia$gpresentazione di Franca Restuccia 210 $aRoma$cGangemi$dstampa 2002 215 $a126 p.$cill.$d30 cm. 410 1$1001SUN0018204$12001 $aDocumenti$v19$1210 $aRoma$cGangemi. 620 $dRoma$3SUNL000360 700 1$aGalizia$b, Mariateresa$3SUNV048067$0496870 702 1$aRestuccia$b, Franca$3SUNV013901 712 $aGangemi$3SUNV000237$4650 801 $aIT$bSOL$c20181109$gRICA 912 $aSUN0060929 950 $aBIBLIOTECA DEL DIPARTIMENTO DI ARCHITETTURA E DISEGNO INDUSTRIALE$d01 PREST IBb579 $e01 6382 995 $aBIBLIOTECA DEL DIPARTIMENTO DI ARCHITETTURA E DISEGNO INDUSTRIALE$bIT-CE0107$h6382$kPREST IBb579$op$qa 996 $aAmbiente urbano di Catania nel '900$9750535 997 $aUNICAMPANIA LEADER 03190nam 2200541 450 001 9910793833503321 005 20231110232325.0 010 $a2-7598-2437-3 024 7 $a10.1051/978-2-7598-2437-3 035 $a(CKB)4100000010080752 035 $a(MiAaPQ)EBC6006604 035 $a(DE-B1597)573467 035 $a(DE-B1597)9782759824373 035 $a(OCoLC)1233041673 035 $a(MiAaPQ)EBC6810509 035 $a(Au-PeEL)EBL6810509 035 $a(PPN)242830250 035 $a(EXLCZ)994100000010080752 100 $a20200302d2020 uy 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 00$aMulti-dimensional processes in stellar physics $eEvry Schatzman School 2018 /$fMichel Rieutord, Isabelle Baraffe and Yveline Lebreton, Eds 210 1$a[Place of publication not identified] :$cEDP Sciences,$d[2020] 210 4$d©2020 215 $a1 online resource (230 pages) 225 0 $aEDP sciences proceedings 311 0 $a2-7598-2416-0 320 $aIncludes bibliographical references. 327 $tFront matter --$tList of Participants --$tTable of contents --$tPreface --$tDouble-diffusive processes in stellar astrophysics --$tThermo-compositional adiabatic and diabatic convection --$tFully compressible time implicit hydrodynamics simulations for stellar interiors --$tThermal Convection in Stars and in Their Atmosphere --$tTurbulence in stably stratified radiative zone --$tAn extremely short course on stellar rotation and magnetism --$tStellar magnetism: bridging dynamos and winds --$tMulti-dimensional asteroseismology --$tMulti-dimensional physics of core-collapse supernovae --$tReferences 330 $aWhen one has to deal with fluid flows, magnetic fields or heat transfer in stars, one faces the partial differential equations that govern these processes. These phenomena are naturally multi-dimensional and their study requires new and sophisticated models. This volume gathers the lecture notes which summarize the essence of the lectures and conferences given by world experts in the field of multi-dimensional modelling of stars, during the 2018 Evry Schatzman School held in Roscoff, France. It gives the present status of our understanding of several processes that occur in stars, like thermal convection, double-diffusive convection, dynamo effect or baroclinic flows. Every subject is discussed under the light of the most recent results of nowadays research and is made accessible to all newcomers, either students or researchers who wish to join the field. 410 0$aEDP Sciences Proceedings 606 $aDifferential equations, Partial$vCongresses 615 0$aDifferential equations, Partial 676 $a515.353 700 $aRieutord$b Michel$4aut$4http://id.loc.gov/vocabulary/relators/aut$0792293 702 $aRieutord$b Michel 702 $aBaraffe$b Isabelle 702 $aLebreton$b Yveline 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910793833503321 996 $aMulti-dimensional processes in stellar physics$93688550 997 $aUNINA