東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back

Switch To: Labeled | MARC Mode | ISBD

Fast solar wind driven by parametric...

Shoda, Munehito.

Linked to FindBook

Google Book

Amazon

博客來

Fast solar wind driven by parametric decay instability and Alfven wave turbulence

Record Type:	Electronic resources : Monograph/item
Title/Author:	Fast solar wind driven by parametric decay instability and Alfven wave turbulence/ by Munehito Shoda.
Author:	Shoda, Munehito.
Published:	Singapore :Springer Singapore : : 2021.,
Description:	xv, 94 p. :ill., digital ;24 cm.
[NT 15003449]:	General 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.
Contained By:	Springer Nature eBook
Subject:	Solar wind. -
Online resource:	https://doi.org/10.1007/978-981-16-1030-1
ISBN:	9789811610301

Fast solar wind driven by parametric decay instability and Alfven wave turbulence
Shoda, Munehito.

Fast solar wind driven by parametric decay instability and Alfven wave turbulence[electronic resource] /by Munehito Shoda. - Singapore :Springer Singapore :2021. - xv, 94 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

General 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.

This 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.

ISBN: 9789811610301

Standard No.: 10.1007/978-981-16-1030-1doiSubjects--Topical Terms:

673099
Solar wind.

LC Class. No.: QB529 / .S563 2021

Dewey Class. No.: 523.58

Fast solar wind driven by parametric decay instability and Alfven wave turbulence
LDR:02380nmm a2200337 a 4500 001 2239738
003 DE-He213
005 20210726145054.0
006 m d
007 cr nn 008maaau
008 211111s2021 si s 0 eng d
020 $a 9789811610301 $q (electronic bk.)
020 $a 9789811610295 $q (paper)
024 7 $a 10.1007/978-981-16-1030-1 $2 doi
035 $a 978-981-16-1030-1
040 $a GP $c GP
041 0 $a eng
050 4 $a QB529 $b .S563 2021
072 7 $a RB $2 bicssc
072 7 $a SCI019000 $2 bisacsh
072 7 $a RB $2 thema
082 0 4 $a 523.58 $2 23
090 $a QB529 $b .S559 2021
100 1 $a Shoda, Munehito. $3 3494025
245 1 0 $a Fast solar wind driven by parametric decay instability and Alfven wave turbulence $h [electronic resource] / $c by Munehito Shoda.
260 $a Singapore : $b Springer Singapore : $b Imprint: Springer, $c 2021.
300 $a xv, 94 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a General 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.
520 $a This 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.
650 0 $a Solar wind. $3 673099
650 0 $a Solar wind $x Mathematical models. $3 3494026
650 1 4 $a Earth Sciences, general. $3 1001754
650 2 4 $a Astrophysics and Astroparticles. $3 1067087
650 2 4 $a Astronomy, Astrophysics and Cosmology. $3 890823
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer Nature eBook
830 0 $a Springer theses. $3 1314442
856 4 0 $u https://doi.org/10.1007/978-981-16-1030-1
950 $a Earth and Environmental Science (SpringerNature-11646)