001435947 000__ 03194cam\a2200517\i\4500
001435947 001__ 1435947
001435947 003__ OCoLC
001435947 005__ 20230309004001.0
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001435947 007__ cr\cn\nnnunnun
001435947 008__ 210422s2021\\\\si\a\\\\ob\\\\000\0\eng\d
001435947 020__ $$a9789811610301$$q(electronic bk.)
001435947 020__ $$a9811610304$$q(electronic bk.)
001435947 020__ $$z9789811610295
001435947 0247_ $$a10.1007/978-981-16-1030-1$$2doi
001435947 035__ $$aSP(OCoLC)1247085112
001435947 040__ $$aGW5XE$$beng$$erda$$epn$$cGW5XE$$dOCLCO$$dEBLCP$$dOCLCF$$dUKAHL$$dOCLCQ$$dOCLCO$$dCOM$$dOCLCQ
001435947 049__ $$aISEA
001435947 050_4 $$aQB529
001435947 08204 $$a523.5/8$$223
001435947 1001_ $$aShoda, Munehito,$$eauthor.
001435947 24510 $$aFast solar wind driven by parametric decay instability and Alfvén wave turbulence /$$cMunehito Shoda.
001435947 264_1 $$aSingapore :$$bSpringer,$$c[2021]
001435947 300__ $$a1 online resource (xv, 94 pages) :$$billustrations (chiefly color)
001435947 336__ $$atext$$btxt$$2rdacontent
001435947 337__ $$acomputer$$bc$$2rdamedia
001435947 338__ $$aonline resource$$bcr$$2rdacarrier
001435947 4901_ $$aSpringer theses,$$x2190-5053
001435947 500__ $$a"Doctoral thesis accepted by The University of Tokyo, Tokyo, Japan."
001435947 504__ $$aIncludes bibliographical references.
001435947 5050_ $$aGeneral Introduction -- 1D model with Compressional and Non-compressional Nonlinear Effects -- Onset and Suppression of Parametric Decay Instability -- 3D Simulations of the Fast Solar Wind -- Summary and Discussion.
001435947 506__ $$aAccess limited to authorized users.
001435947 520__ $$aThis book discusses key theoretical aspects concerning the formation of the solar wind: the most essential building block in the heliosphere, in which planets orbit. To understand the influence of solar activity on planetary magnetospheres and atmospheres, we need to first understand the origin of the solar wind, which is still under debate. This book presents the outcomes of state-of-the-art numerical simulations of solar wind acceleration, including the first three-dimensional simulation of the turbulence-driven solar wind model. One of the book's goals is to include compressional effects in the dynamics of solar wind turbulence; accordingly, it discusses parametric decay instability in detail. Several key aspects that are relevant to the Parker Solar Probe observations are also discussed. Given its scope, the book plays a key role in bridging the gap between the theory of magnetohydrodynamic turbulence and current/future in-situ observations of the solar wind. This book is based on the Ph. D. thesis by the author, which won the 2019 International Astronomical Union Division E Ph. D. prize.
001435947 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed April 22, 2021).
001435947 650_0 $$aSolar wind.
001435947 650_0 $$aSolar wind$$xMathematical models.
001435947 650_6 $$aVents solaires.
001435947 650_6 $$aVents solaires$$xModèles mathématiques.
001435947 655_0 $$aElectronic books.
001435947 830_0 $$aSpringer theses.$$x2190-5053
001435947 852__ $$bebk
001435947 85640 $$3Springer Nature$$uhttps://univsouthin.idm.oclc.org/login?url=https://link.springer.com/10.1007/978-981-16-1030-1$$zOnline Access$$91397441.1
001435947 909CO $$ooai:library.usi.edu:1435947$$pGLOBAL_SET
001435947 980__ $$aBIB
001435947 980__ $$aEBOOK
001435947 982__ $$aEbook
001435947 983__ $$aOnline
001435947 994__ $$a92$$bISE