大葉大學圖書館 |

The strongest magnetic fields in the universe[electronic resource] /

レコード種別:	言語・文字資料 (印刷物) : 単行資料
[NT 15000414] null:	523.0188
タイトル / 著者:	The strongest magnetic fields in the universe/ edited by V.S. Beskin ... [et al.].
その他の著者:	Beskin, V.S.
出版された:	New York, NY : : Springer New York :, 2016.
記述:	x, 583 p. : : ill. (some col.), digital ;; 24 cm.
含まれています:	Springer eBooks
主題:	Cosmic magnetic fields.
主題:	Physics.
主題:	Extraterrestrial Physics, Space Sciences.
主題:	Cosmology.
主題:	Magnetism, Magnetic Materials.
国際標準図書番号 (ISBN) :	9781493935505
国際標準図書番号 (ISBN) :	9781493935499
[NT 15000228] null:	Foreword -- Part I: Introduction -- Magnetic Fields at Largest Universal Strengths: Overview -- Physics in Very Strong Magnetic Fields: An Introduction -- Part II: Magnetic Fields in Stars -- Observations of Strong Magnetic Fields in Nondegenerate Stars -- Magnetic Field Generation in Stars -- Magnetic White Dwarfs -- Part III: Neutron Stars -- Neutron Stars: Thermal Emitters -- Radio Pulsars -- Neutron Stars: Cooling and Transport -- Magnetic Fields of Neutron Stars in X-ray Binaries -- Magnetars: Properties, Origin and Evolution -- Part IV: Accretion, Winds, Jets -- Accretion and Outflows from Magnetized Stars -- Pulsar Wind Nebulae -- Disks and Jets: Gravity, Rotation and Magnetic Fields -- Part V: Physical Processes -- Gamma Ray Bursts As Sources of Strong Magnetic Fields -- Relativistic Shocks Particle Acceleration and Magnetization -- Relativistic Magnetic Reconnection and Its Astrophysical Applications.
[NT 15000229] null:	This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, degenerate stars (such as white dwarfs and neutron stars), exotic members called magnetars, and in their environments, as well as magnetic fields in the environments of black holes. These strong fields have a profound effect on the behavior of matter, visible in particular in highly variable processes like radiation in all known wavelengths, including Gamma-Ray bursts. The generation and structure of such strong magnetic fields and effects on the environment are also described.
電子資源:	http://dx.doi.org/10.1007/978-1-4939-3550-5

The strongest magnetic fields in the universe[electronic resource] /
The strongest magnetic fields in the universe[electronic resource] /edited by V.S. Beskin ... [et al.]. - New York, NY :Springer New York :2016. - x, 583 p. :ill. (some col.), digital ;24 cm. - Space sciences series of ISSI,v.541385-7525 ;. - Space sciences series of ISSI ;v.37..

Foreword -- Part I: Introduction -- Magnetic Fields at Largest Universal Strengths: Overview -- Physics in Very Strong Magnetic Fields: An Introduction -- Part II: Magnetic Fields in Stars -- Observations of Strong Magnetic Fields in Nondegenerate Stars -- Magnetic Field Generation in Stars -- Magnetic White Dwarfs -- Part III: Neutron Stars -- Neutron Stars: Thermal Emitters -- Radio Pulsars -- Neutron Stars: Cooling and Transport -- Magnetic Fields of Neutron Stars in X-ray Binaries -- Magnetars: Properties, Origin and Evolution -- Part IV: Accretion, Winds, Jets -- Accretion and Outflows from Magnetized Stars -- Pulsar Wind Nebulae -- Disks and Jets: Gravity, Rotation and Magnetic Fields -- Part V: Physical Processes -- Gamma Ray Bursts As Sources of Strong Magnetic Fields -- Relativistic Shocks Particle Acceleration and Magnetization -- Relativistic Magnetic Reconnection and Its Astrophysical Applications.

This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, degenerate stars (such as white dwarfs and neutron stars), exotic members called magnetars, and in their environments, as well as magnetic fields in the environments of black holes. These strong fields have a profound effect on the behavior of matter, visible in particular in highly variable processes like radiation in all known wavelengths, including Gamma-Ray bursts. The generation and structure of such strong magnetic fields and effects on the environment are also described.

ISBN: 9781493935505

Standard No.: 10.1007/978-1-4939-3550-5doiSubjects--Topical Terms:

605096
Cosmic magnetic fields.

LC Class. No.: QC809.M25

Dewey Class. No.: 523.0188

The strongest magnetic fields in the universe[electronic resource] /
LDR:02725nam a2200325 a 4500 001 456410
003 DE-He213
005 20160818141519.0
006 m d
007 cr nn 008maaau
008 161227s2016 nyu s 0 eng d
020 $a 9781493935505 $q (electronic bk.)
020 $a 9781493935499 $q (paper)
024 7 $a 10.1007/978-1-4939-3550-5 $2 doi
035 $a 978-1-4939-3550-5
040 $a GP $c GP
041 0 $a eng
050 4 $a QC809.M25
072 7 $a TTDS $2 bicssc
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 523.0188 $2 23
090 $a QC809.M25 $b S924 2016
245 1 4 $a The strongest magnetic fields in the universe $h [electronic resource] / $c edited by V.S. Beskin ... [et al.].
260 $a New York, NY : $b Springer New York : $b Imprint: Springer, $c 2016.
300 $a x, 583 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Space sciences series of ISSI, $x 1385-7525 ; $v v.54
505 0 $a Foreword -- Part I: Introduction -- Magnetic Fields at Largest Universal Strengths: Overview -- Physics in Very Strong Magnetic Fields: An Introduction -- Part II: Magnetic Fields in Stars -- Observations of Strong Magnetic Fields in Nondegenerate Stars -- Magnetic Field Generation in Stars -- Magnetic White Dwarfs -- Part III: Neutron Stars -- Neutron Stars: Thermal Emitters -- Radio Pulsars -- Neutron Stars: Cooling and Transport -- Magnetic Fields of Neutron Stars in X-ray Binaries -- Magnetars: Properties, Origin and Evolution -- Part IV: Accretion, Winds, Jets -- Accretion and Outflows from Magnetized Stars -- Pulsar Wind Nebulae -- Disks and Jets: Gravity, Rotation and Magnetic Fields -- Part V: Physical Processes -- Gamma Ray Bursts As Sources of Strong Magnetic Fields -- Relativistic Shocks Particle Acceleration and Magnetization -- Relativistic Magnetic Reconnection and Its Astrophysical Applications.
520 $a This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, degenerate stars (such as white dwarfs and neutron stars), exotic members called magnetars, and in their environments, as well as magnetic fields in the environments of black holes. These strong fields have a profound effect on the behavior of matter, visible in particular in highly variable processes like radiation in all known wavelengths, including Gamma-Ray bursts. The generation and structure of such strong magnetic fields and effects on the environment are also described.
650 0 $a Cosmic magnetic fields. $3 605096
650 1 4 $a Physics. $3 171863
650 2 4 $a Extraterrestrial Physics, Space Sciences. $3 464218
650 2 4 $a Cosmology. $3 395561
650 2 4 $a Magnetism, Magnetic Materials. $3 463743
700 1 $a Beskin, V.S. $3 655781
710 2 $a SpringerLink (Online service) $3 463450
773 0 $t Springer eBooks
830 0 $a Space sciences series of ISSI ; $v v.37. $3 468608
856 4 0 $u http://dx.doi.org/10.1007/978-1-4939-3550-5
950 $a Physics and Astronomy (Springer-11651)