國立高雄大學圖資館 |

語系: 繁體中文

說明(常見問題)

圖資館首頁

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Dawn-dusk asymmetries in planetary p...

Forsyth, Colin.

Dawn-dusk asymmetries in planetary plasma environments

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Dawn-dusk asymmetries in planetary plasma environmentsStein Haaland, Andrei Runov, Colin Forsyth, editors.
其他作者:	Haaland, Stein.
出版者:	Hoboken, NJ :John Wiley & Sons ;2017.
面頁冊數:	1 online resource (360 p.)
附註:	"This work is a co-publication of the American Geophysical Union and John Wiley and Sons, Inc."
標題:	Magnetosphere.
電子資源:	https://onlinelibrary.wiley.com/doi/book/10.1002/9781119216346
ISBN:	9781119216346$q(electronic bk.)

Dawn-dusk asymmetries in planetary plasma environments
Dawn-dusk asymmetries in planetary plasma environments[electronic resource] /Stein Haaland, Andrei Runov, Colin Forsyth, editors. - 1st ed. - Hoboken, NJ :John Wiley & Sons ;2017. - 1 online resource (360 p.) - Geophysical monograph series ;230. - Geophysical monograph series ;207..

"This work is a co-publication of the American Geophysical Union and John Wiley and Sons, Inc."

Includes bibliographical references and index.

"Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other. For example, recent observations indicate that Earth's magnetopause is thicker at dawn than at dusk. Likewise, auroral breakups at Earth are more likely to occur in the pre-midnight than post-midnight sectors. Increasing availability of remotely sensed and in situ measurements of planetary ionospheres, magnetospheres and their interfaces to the solar wind have revealed significant and persistent dawn-dusk asymmetries. As yet there is no consensus regarding the source of many of these asymmetries, nor the physical mechanisms by which they are produced and maintained. Volume highlights include: A comprehensive and updated overview of current knowledge about dawn-dusk asymmetries in the plasma environments of planets in our solar system and the mechanisms behind them; Valuable contributions from internationally recognized experts, covering both observations, simulations and theories discussing all important aspects of dawn-dusk asymmetries; Space weather effects are caused by processes in space, mainly the magnetotail, and can be highly localized on ground. Knowing where the source, i.e., where dawn-dusk location is will allow for a better prediction of where the effects on ground will be most pronounced" -- Provided by publisher.

ISBN: 9781119216346$q(electronic bk.)Subjects--Topical Terms:

339222
Magnetosphere.

LC Class. No.: QC809.M35

Dewey Class. No.: 538.766

Dawn-dusk asymmetries in planetary plasma environments
LDR:02785cmm a2200349 a 4500 001 536894
003 OCoLC
005 20180330091358.2
006 m o d
007 cr |n|||||||||
008 190109s2017 nju o 000 0 eng d
020 $a 9781119216346$q(electronic bk.)
020 $a 1119216346$q(electronic bk.)
020 $a 9781119216513$q(electronic bk.)
020 $a 1119216516$q(electronic bk.)
020 $a 9781119216353
020 $a 1119216354
020 $z 9781119216322
020 $z 111921632X
035 $a 1005887871
040 $a YDX $b eng $c YDX $d N $d EBLCP $d N $d DG1 $d OCLCF $d MERER $d OCLCQ $d UAB $d UPM $d MEU $d NLE $d OCLCQ
050 4 $a QC809.M35
082 0 $a 538.766
245 0 0 $a Dawn-dusk asymmetries in planetary plasma environments $h [electronic resource] / $c Stein Haaland, Andrei Runov, Colin Forsyth, editors.
250 $a 1st ed.
260 $a Hoboken, NJ : $b John Wiley & Sons ; $a Washington, D.C. : $b American Geophysical Union, $c 2017.
300 $a 1 online resource (360 p.)
490 1 $a Geophysical monograph series ; $v 230
500 $a "This work is a co-publication of the American Geophysical Union and John Wiley and Sons, Inc."
504 $a Includes bibliographical references and index.
520 $a "Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other. For example, recent observations indicate that Earth's magnetopause is thicker at dawn than at dusk. Likewise, auroral breakups at Earth are more likely to occur in the pre-midnight than post-midnight sectors. Increasing availability of remotely sensed and in situ measurements of planetary ionospheres, magnetospheres and their interfaces to the solar wind have revealed significant and persistent dawn-dusk asymmetries. As yet there is no consensus regarding the source of many of these asymmetries, nor the physical mechanisms by which they are produced and maintained. Volume highlights include: A comprehensive and updated overview of current knowledge about dawn-dusk asymmetries in the plasma environments of planets in our solar system and the mechanisms behind them; Valuable contributions from internationally recognized experts, covering both observations, simulations and theories discussing all important aspects of dawn-dusk asymmetries; Space weather effects are caused by processes in space, mainly the magnetotail, and can be highly localized on ground. Knowing where the source, i.e., where dawn-dusk location is will allow for a better prediction of where the effects on ground will be most pronounced" -- Provided by publisher.
588 $a Description based on print version record.
650 0 $a Magnetosphere. $3 339222
700 1 $a Haaland, Stein. $3 813421
700 1 $a Runov, Andrei. $3 813422
700 1 $a Forsyth, Colin. $3 813423
830 0 $a Geophysical monograph series ; $v 207. $3 721606
856 4 0 $u https://onlinelibrary.wiley.com/doi/book/10.1002/9781119216346