國立虎尾科技大學 |

Interactions of Earth's magnetotail plasma with the surface, plasma, and magnetic anomalies of the moon

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Interactions of Earth's magnetotail plasma with the surface, plasma, and magnetic anomalies of the moon/ by Yuki Harada.
作者:	Harada, Yuki.
出版者:	Tokyo :Springer Japan : : 2015.,
面頁冊數:	xiii, 111 p. :ill. (some col.), digital ; : 24 cm.;
Contained By:	Springer eBooks
標題:	Space plasmas. -
電子資源:	http://dx.doi.org/10.1007/978-4-431-55084-6
ISBN:	9784431550846 (electronic bk.)

Interactions of Earth's magnetotail plasma with the surface, plasma, and magnetic anomalies of the moon
Harada, Yuki.

Interactions of Earth's magnetotail plasma with the surface, plasma, and magnetic anomalies of the moon[electronic resource] /by Yuki Harada. - Tokyo :Springer Japan :2015. - xiii, 111 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Electron Gyro-scale Dynamics near the Lunar Surface -- Lunar Dayside Plasma in the Earth's Magnetotail Lobes -- Hot-Proton Interactions with the Surface and Magnetic Anomalies of the Moon -- Conclusions.

This thesis describes the essential features of Moon-plasma interactions with a particular emphasis on the Earth's magnetotail plasma regime from both observational and theoretical standpoints. The Moon lacks a dense atmosphere as well as a strong intrinsic magnetic field. As a result, its interactions with the ambient plasma are drastically different from solar-wind interactions with magnetized planets such as Earth. The Moon encounters a wide range of plasma regime from the relatively dense, cold, supersonic solar-wind plasma to the low-density, hot, subsonic plasma in the geomagnetic tail. In this book, the author presents a series of new observations from recent lunar missions (i.e., Kaguya, ARTEMIS, and Chandrayaan-1), demonstrating the importance of the electron gyro-scale dynamics, plasma of lunar origin, and hot plasma interactions with lunar magnetic anomalies. The similarity and difference between the Moon-plasma interactions in the geomagnetic tail and those in the solar wind are discussed throughout the thesis. The basic knowledge presented in this book can be applied to plasma interactions with airless bodies throughout the solar system and beyond.

ISBN: 9784431550846 (electronic bk.)

Standard No.: 10.1007/978-4-431-55084-6doiSubjects--Topical Terms:

782557
Space plasmas.

LC Class. No.: QC809.P5

Dewey Class. No.: 523.01

Interactions of Earth's magnetotail plasma with the surface, plasma, and magnetic anomalies of the moon
LDR:02442nam a2200325 a 4500 001 834161
003 DE-He213
005 20150518145233.0
006 m d
007 cr nn 008maaau
008 160421s2015 ja s 0 eng d
020 $a 9784431550846 (electronic bk.)
020 $a 9784431550839 (paper)
024 7 $a 10.1007/978-4-431-55084-6 $2 doi
035 $a 978-4-431-55084-6
040 $a GP $c GP
041 0 $a eng
050 4 $a QC809.P5
072 7 $a PHVG $2 bicssc
072 7 $a SCI032000 $2 bisacsh
082 0 4 $a 523.01 $2 23
090 $a QC809.P5 $b H254 2015
100 1 $a Harada, Yuki. $3 1062409
245 1 0 $a Interactions of Earth's magnetotail plasma with the surface, plasma, and magnetic anomalies of the moon $h [electronic resource] / $c by Yuki Harada.
260 $a Tokyo : $c 2015. $b Springer Japan : $b Imprint: Springer,
300 $a xiii, 111 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- Electron Gyro-scale Dynamics near the Lunar Surface -- Lunar Dayside Plasma in the Earth's Magnetotail Lobes -- Hot-Proton Interactions with the Surface and Magnetic Anomalies of the Moon -- Conclusions.
520 $a This thesis describes the essential features of Moon-plasma interactions with a particular emphasis on the Earth's magnetotail plasma regime from both observational and theoretical standpoints. The Moon lacks a dense atmosphere as well as a strong intrinsic magnetic field. As a result, its interactions with the ambient plasma are drastically different from solar-wind interactions with magnetized planets such as Earth. The Moon encounters a wide range of plasma regime from the relatively dense, cold, supersonic solar-wind plasma to the low-density, hot, subsonic plasma in the geomagnetic tail. In this book, the author presents a series of new observations from recent lunar missions (i.e., Kaguya, ARTEMIS, and Chandrayaan-1), demonstrating the importance of the electron gyro-scale dynamics, plasma of lunar origin, and hot plasma interactions with lunar magnetic anomalies. The similarity and difference between the Moon-plasma interactions in the geomagnetic tail and those in the solar wind are discussed throughout the thesis. The basic knowledge presented in this book can be applied to plasma interactions with airless bodies throughout the solar system and beyond.
650 0 $a Space plasmas. $3 782557
650 0 $a Plasma astrophysics. $3 890950
650 1 4 $a Earth Sciences. $3 683879
650 2 4 $a Geophysics/Geodesy. $3 668510
650 2 4 $a Extraterrestrial Physics, Space Sciences. $3 669918
650 2 4 $a Planetology. $3 593937
650 2 4 $a Astrophysics and Astroparticles. $3 782546
710 2 $a SpringerLink (Online service) $3 593884
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 831604
856 4 0 $u http://dx.doi.org/10.1007/978-4-431-55084-6
950 $a Earth and Environmental Science (Springer-11646)