東華大學圖書館 |

語系: 繁體中文

說明(常見問題)

回圖書館首頁

手機版館藏查詢

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

FindBook

Google Book

Amazon

博客來

Solar rotation

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Solar rotation/ by Roman Brajša, Arnold Hanslmeier.
作者:	Brajša, Roman.
其他作者:	Hanslmeier, Arnold.
出版者:	Singapore :Springer Nature Singapore : : 2024.,
面頁冊數:	xvi, 180 p. :ill. (some col.), digital ;24 cm.
內容註:	The Sun as a star: fundamental properties -- Solar rotation elements -- Coordinate systems and coordinate transformation -- Methods for solar rotation measurements -- Analysis and reduction of observational data -- A comparison of various observational results of solar differential rotation -- Solar rotation and activity -- Literature.
Contained By:	Springer Nature eBook
標題:	Solar Physics. -
標題:	Sun - Rotation. -
電子資源:	https://doi.org/10.1007/978-981-97-6879-0
ISBN:	9789819768790

Solar rotation
Brajša, Roman.

Solar rotation[electronic resource] /by Roman Brajša, Arnold Hanslmeier. - Singapore :Springer Nature Singapore :2024. - xvi, 180 p. :ill. (some col.), digital ;24 cm. - UNITEXT for physics,2198-7890. - UNITEXT for physics..

The Sun as a star: fundamental properties -- Solar rotation elements -- Coordinate systems and coordinate transformation -- Methods for solar rotation measurements -- Analysis and reduction of observational data -- A comparison of various observational results of solar differential rotation -- Solar rotation and activity -- Literature.

The rotation of the Sun is a basic parameter which constrains the boundary conditions for the model of the MHD-dynamo mechanisms that generates solar activity. The Sun is a slowly rotating star with a convection zone below the surface which is the site of the solar dynamo. The solar rotation depends on the latitude, depth/height and time, i.e., the Sun rotates differentially. In the book several aspects of the solar rotation are covered. Only in the case of the Sun we can directly observe details in its atmosphere and so measure the rotation velocity using various tracers, which is one of the mostly used methods for rotation determination. So, the Sun is a prototype for studying other stars. Different techniques that enable to determine solar rotation (e.g., tracer method, spectroscopic method, helioseismology) are presented and their results are compared and interpreted. In the current literature there is no book exclusively about solar rotation published in the last several decades. The book is intended for astrophysicists, both professionals as well as students and people interested in science in general. The reader would strongly benefit from the comprehensive description of several topics related to the solar rotation. The authors are highly experienced in teaching astrophysics both to astrophysicists, solar physicists as well as to the public. Therefore, from the didactical point of view the book is written basically as a textbook, so the reader that is not deep within that field can gain an overview. Moreover, for those who want to get deeper into the topics, additional information is given, and recommendations for further literature as well as many citations to recent publications. The reader will get both (i) a general introduction into the topics (ii) overview of recent publications on the topics. Therefore, the book can serve as a textbook but will be also very useful for research and thesis writing, for example.

ISBN: 9789819768790

Standard No.: 10.1007/978-981-97-6879-0doiSubjects--Topical Terms:

3603457
Solar Physics.
Subjects--Geographical Terms:

3735258
Sun
--Rotation.

LC Class. No.: QB523

Dewey Class. No.: 523.73

Solar rotation
LDR:03301nmm a2200337 a 4500 001 2381255
003 DE-He213
005 20241130115256.0
006 m d
007 cr nn 008maaau
008 250418s2024 si s 0 eng d
020 $a 9789819768790 $q (electronic bk.)
020 $a 9789819768783 $q (paper)
024 7 $a 10.1007/978-981-97-6879-0 $2 doi
035 $a 978-981-97-6879-0
040 $a GP $c GP
041 0 $a eng
050 4 $a QB523
072 7 $a PGS $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PGS $2 thema
082 0 4 $a 523.73 $2 23
090 $a QB523 $b .B814 2024
100 1 $a Brajša, Roman. $3 3719591
245 1 0 $a Solar rotation $h [electronic resource] / $c by Roman Brajša, Arnold Hanslmeier.
260 $a Singapore : $b Springer Nature Singapore : $b Imprint: Springer, $c 2024.
300 $a xvi, 180 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a UNITEXT for physics, $x 2198-7890
505 0 $a The Sun as a star: fundamental properties -- Solar rotation elements -- Coordinate systems and coordinate transformation -- Methods for solar rotation measurements -- Analysis and reduction of observational data -- A comparison of various observational results of solar differential rotation -- Solar rotation and activity -- Literature.
520 $a The rotation of the Sun is a basic parameter which constrains the boundary conditions for the model of the MHD-dynamo mechanisms that generates solar activity. The Sun is a slowly rotating star with a convection zone below the surface which is the site of the solar dynamo. The solar rotation depends on the latitude, depth/height and time, i.e., the Sun rotates differentially. In the book several aspects of the solar rotation are covered. Only in the case of the Sun we can directly observe details in its atmosphere and so measure the rotation velocity using various tracers, which is one of the mostly used methods for rotation determination. So, the Sun is a prototype for studying other stars. Different techniques that enable to determine solar rotation (e.g., tracer method, spectroscopic method, helioseismology) are presented and their results are compared and interpreted. In the current literature there is no book exclusively about solar rotation published in the last several decades. The book is intended for astrophysicists, both professionals as well as students and people interested in science in general. The reader would strongly benefit from the comprehensive description of several topics related to the solar rotation. The authors are highly experienced in teaching astrophysics both to astrophysicists, solar physicists as well as to the public. Therefore, from the didactical point of view the book is written basically as a textbook, so the reader that is not deep within that field can gain an overview. Moreover, for those who want to get deeper into the topics, additional information is given, and recommendations for further literature as well as many citations to recent publications. The reader will get both (i) a general introduction into the topics (ii) overview of recent publications on the topics. Therefore, the book can serve as a textbook but will be also very useful for research and thesis writing, for example.
650 1 4 $a Solar Physics. $3 3603457
650 2 4 $a Thermodynamics. $3 517304
650 2 4 $a Astrophysics. $3 535904
650 2 4 $a Space Physics. $3 3538914
650 2 4 $a Cosmology. $3 531904
650 2 4 $a Plasma Physics. $3 1074160
651 0 $a Sun $x Rotation. $3 3735258
700 1 $a Hanslmeier, Arnold. $3 817382
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer Nature eBook
830 0 $a UNITEXT for physics. $3 2068732
856 4 0 $u https://doi.org/10.1007/978-981-97-6879-0
950 $a Physics and Astronomy (SpringerNature-11651)