語系:
繁體中文
English
說明(常見問題)
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Study on Magnetohydrodynamic Turbule...
~
Xu, Siyao.
Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications
紀錄類型:
書目-語言資料,印刷品 : Monograph/item
正題名/作者:
Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications/ by Siyao Xu.
作者:
Xu, Siyao.
面頁冊數:
XIII, 157 p. 13 illus., 3 illus. in color.online resource. :
Contained By:
Springer Nature eBook
標題:
Astrophysics. -
電子資源:
https://doi.org/10.1007/978-981-13-7515-6
ISBN:
9789811375156
Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications
Xu, Siyao.
Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications
[electronic resource] /by Siyao Xu. - 1st ed. 2019. - XIII, 157 p. 13 illus., 3 illus. in color.online resource. - Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053. - Springer Theses, Recognizing Outstanding Ph.D. Research,.
Turbulence and magnetic fields are ubiquitous in the Universe. Their importance to astronomy cannot be overestimated. The theoretical advancements in magnetohydrodynamic (MHD) turbulence achieved during the past two decades have significantly influenced many fields of astronomy. This book provides predictive theories of the magnetic field generation by turbulence and the dissipation of MHD turbulence. These fundamental non-linear problems were believed to be tractable only numerically. This book provides complete analytical descriptions in quantitative agreement with existing numerics, as well as theoretical predictions in physical regimes still unreachable by simulations, and explanations of various related observations. It also discusses and promotes the astrophysical applications of MHD turbulence theories, including (i) the particle acceleration and radiation in high-energy phenomena, e.g., Gamma-Ray Bursts, supernova remnants, cosmic rays; (ii) interstellar density fluctuations and the effect on observations, e.g., Faraday rotation, scattering measurements of Galactic and extragalactic radio sources; (iii) density and magnetic field structure in molecular clouds toward star formation. In closing, this book demonstrates the key role of MHD turbulence in connecting diverse astrophysical processes and unraveling long-standing astrophysical problems, as foreseen by Chandrasekhar, a founder of modern astrophysics.
ISBN: 9789811375156
Standard No.: 10.1007/978-981-13-7515-6doiSubjects--Topical Terms:
646223
Astrophysics.
LC Class. No.: QB460-466
Dewey Class. No.: 523.01
Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications
LDR
:02862nam a22003975i 4500
001
1009752
003
DE-He213
005
20200702170752.0
007
cr nn 008mamaa
008
210106s2019 si | s |||| 0|eng d
020
$a
9789811375156
$9
978-981-13-7515-6
024
7
$a
10.1007/978-981-13-7515-6
$2
doi
035
$a
978-981-13-7515-6
050
4
$a
QB460-466
072
7
$a
PHVB
$2
bicssc
072
7
$a
SCI005000
$2
bisacsh
072
7
$a
PHVB
$2
thema
082
0 4
$a
523.01
$2
23
100
1
$a
Xu, Siyao.
$4
aut
$4
http://id.loc.gov/vocabulary/relators/aut
$3
1226265
245
1 0
$a
Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications
$h
[electronic resource] /
$c
by Siyao Xu.
250
$a
1st ed. 2019.
264
1
$a
Singapore :
$b
Springer Singapore :
$b
Imprint: Springer,
$c
2019.
300
$a
XIII, 157 p. 13 illus., 3 illus. in color.
$b
online resource.
336
$a
text
$b
txt
$2
rdacontent
337
$a
computer
$b
c
$2
rdamedia
338
$a
online resource
$b
cr
$2
rdacarrier
347
$a
text file
$b
PDF
$2
rda
490
1
$a
Springer Theses, Recognizing Outstanding Ph.D. Research,
$x
2190-5053
520
$a
Turbulence and magnetic fields are ubiquitous in the Universe. Their importance to astronomy cannot be overestimated. The theoretical advancements in magnetohydrodynamic (MHD) turbulence achieved during the past two decades have significantly influenced many fields of astronomy. This book provides predictive theories of the magnetic field generation by turbulence and the dissipation of MHD turbulence. These fundamental non-linear problems were believed to be tractable only numerically. This book provides complete analytical descriptions in quantitative agreement with existing numerics, as well as theoretical predictions in physical regimes still unreachable by simulations, and explanations of various related observations. It also discusses and promotes the astrophysical applications of MHD turbulence theories, including (i) the particle acceleration and radiation in high-energy phenomena, e.g., Gamma-Ray Bursts, supernova remnants, cosmic rays; (ii) interstellar density fluctuations and the effect on observations, e.g., Faraday rotation, scattering measurements of Galactic and extragalactic radio sources; (iii) density and magnetic field structure in molecular clouds toward star formation. In closing, this book demonstrates the key role of MHD turbulence in connecting diverse astrophysical processes and unraveling long-standing astrophysical problems, as foreseen by Chandrasekhar, a founder of modern astrophysics.
650
0
$a
Astrophysics.
$3
646223
650
0
$a
Plasma (Ionized gases).
$3
1253465
650
0
$a
Observations, Astronomical.
$3
1254353
650
0
$a
Astronomy—Observations.
$3
1254354
650
1 4
$a
Astrophysics and Astroparticles.
$3
782546
650
2 4
$a
Plasma Physics.
$3
768744
650
2 4
$a
Astronomy, Observations and Techniques.
$3
769023
710
2
$a
SpringerLink (Online service)
$3
593884
773
0
$t
Springer Nature eBook
776
0 8
$i
Printed edition:
$z
9789811375149
776
0 8
$i
Printed edition:
$z
9789811375163
776
0 8
$i
Printed edition:
$z
9789811375170
830
0
$a
Springer Theses, Recognizing Outstanding Ph.D. Research,
$x
2190-5053
$3
1253569
856
4 0
$u
https://doi.org/10.1007/978-981-13-7515-6
912
$a
ZDB-2-PHA
912
$a
ZDB-2-SXP
950
$a
Physics and Astronomy (SpringerNature-11651)
950
$a
Physics and Astronomy (R0) (SpringerNature-43715)
筆 0 讀者評論
多媒體
評論
新增評論
分享你的心得
Export
取書館別
處理中
...
變更密碼[密碼必須為2種組合(英文和數字)及長度為10碼以上]
登入