國立高雄大學圖資館 |

登入

回首頁

Eruptions on the sun

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Eruptions on the sunby Boris Filippov.
作者:	Filippov, Boris.
出版者:	Cham :Springer Nature Switzerland :2024.
面頁冊數:	x, 393 p. :ill. (chiefly col.), digital ;24 cm.
Contained By:	Springer Nature eBook
標題:	Solar activity.
電子資源:	https://doi.org/10.1007/978-3-031-58177-9
ISBN:	9783031581779$q(electronic bk.)

Eruptions on the sun
Filippov, Boris.

Eruptions on the sun[electronic resource] /by Boris Filippov. - Cham :Springer Nature Switzerland :2024. - x, 393 p. :ill. (chiefly col.), digital ;24 cm. - Astrophysics and space science library,v. 4712214-7985 ;. - Astrophysics and space science library ;379..

Introduction -- General Characteristics of the Sun -- Magnetic Fields on the Sun -- Equilibrium Plasma Structures in the Solar Atmosphere -- Intimate relationship between plasma structures and magnetic fields in the solar atmosphere -- Peculiarities of the Filament Visual Interaction on the Solar Disk -- Eruption of Prominences -- Causes of prominence eruptions -- Solar Jets -- Solar Flares -- Coronal Mass Ejections -- Solar Wind and Space Weather.

This book is devoted to eruptive phenomena on the Sun, the most dangerous sources of space weather disturbances. It discusses the latest achievements in this field, described in the scientific literature and obtained by the author himself. The initial chapters of the book give a brief description of the role of the Sun in the life and history of mankind, a general description of the solar interior and the atmosphere of the Sun, the causes and drivers of solar activity and its impact on the Earth's environment and human life. The book provides a detailed description of eruptive phenomena on the Sun, a review of observations of solar activity and theoretical ideas about the mechanisms and causes of a sudden release of energy in the solar atmosphere. Much attention is paid to the solar magnetic fields, their characteristic features and measured values in the photosphere, the observed manifestations in the chromosphere and corona, and methods for extrapolating photospheric data to the upper layers of the solar atmosphere. It is assumed that the magnetic field is the source of energy suddenly released during eruptive phenomena observed in the form of flares, prominence eruptions and coronal mass ejections (CMEs) Energy is accumulated and stored in the non-potential (associated with electric currents) part of the coronal magnetic field (free magnetic energy) This part of the field is the most variable and can provide energy for fast eruptive processes. CMEs, propagating through the interplanetary medium, significantly perturb it and cause the strongest geomagnetic storms when they affect the Earth's magnetosphere. The prediction of the arrival of the CME is the key problem of the entire space weather forecast. Thus, pre-eruptive conditions in CME source regions are of great importance. Solar prominences and filaments are considered the most likely progenitors of CMEs. Most of the book is devoted to the description and analysis of their equilibrium and stability. It is shown that there are measurable characteristics of the proximity of the prominence to the instability threshold, which can be very useful in the problem of space weather forecasting. The book contains many illustrations and links to the latest scientific articles and reviews on the topic. It will be useful to researchers in the field of astrophysics, solar physics, geophysics, as well as PhD and graduate students.

ISBN: 9783031581779$q(electronic bk.)

Standard No.: 10.1007/978-3-031-58177-9doiSubjects--Topical Terms:

276016
Solar activity.

LC Class. No.: QB524

Dewey Class. No.: 523.7

Eruptions on the sun
LDR:03884nmm a2200337 a 4500 001 658588
003 DE-He213
005 20240629125227.0
006 m d
007 cr nn 008maaau
008 240923s2024 sz s 0 eng d
020 $a 9783031581779$q(electronic bk.)
020 $a 9783031581762$q(paper)
024 7 $a 10.1007/978-3-031-58177-9 $2 doi
035 $a 978-3-031-58177-9
040 $a GP $c GP
041 0 $a eng
050 4 $a QB524
072 7 $a PGS $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PGS $2 thema
082 0 4 $a 523.7 $2 23
090 $a QB524 $b .F483 2024
100 1 $a Filippov, Boris. $3 969805
245 1 0 $a Eruptions on the sun $h [electronic resource] / $c by Boris Filippov.
260 $a Cham : $b Springer Nature Switzerland : $b Imprint: Springer, $c 2024.
300 $a x, 393 p. : $b ill. (chiefly col.), digital ; $c 24 cm.
490 1 $a Astrophysics and space science library, $x 2214-7985 ; $v v. 471
505 0 $a Introduction -- General Characteristics of the Sun -- Magnetic Fields on the Sun -- Equilibrium Plasma Structures in the Solar Atmosphere -- Intimate relationship between plasma structures and magnetic fields in the solar atmosphere -- Peculiarities of the Filament Visual Interaction on the Solar Disk -- Eruption of Prominences -- Causes of prominence eruptions -- Solar Jets -- Solar Flares -- Coronal Mass Ejections -- Solar Wind and Space Weather.
520 $a This book is devoted to eruptive phenomena on the Sun, the most dangerous sources of space weather disturbances. It discusses the latest achievements in this field, described in the scientific literature and obtained by the author himself. The initial chapters of the book give a brief description of the role of the Sun in the life and history of mankind, a general description of the solar interior and the atmosphere of the Sun, the causes and drivers of solar activity and its impact on the Earth's environment and human life. The book provides a detailed description of eruptive phenomena on the Sun, a review of observations of solar activity and theoretical ideas about the mechanisms and causes of a sudden release of energy in the solar atmosphere. Much attention is paid to the solar magnetic fields, their characteristic features and measured values in the photosphere, the observed manifestations in the chromosphere and corona, and methods for extrapolating photospheric data to the upper layers of the solar atmosphere. It is assumed that the magnetic field is the source of energy suddenly released during eruptive phenomena observed in the form of flares, prominence eruptions and coronal mass ejections (CMEs) Energy is accumulated and stored in the non-potential (associated with electric currents) part of the coronal magnetic field (free magnetic energy) This part of the field is the most variable and can provide energy for fast eruptive processes. CMEs, propagating through the interplanetary medium, significantly perturb it and cause the strongest geomagnetic storms when they affect the Earth's magnetosphere. The prediction of the arrival of the CME is the key problem of the entire space weather forecast. Thus, pre-eruptive conditions in CME source regions are of great importance. Solar prominences and filaments are considered the most likely progenitors of CMEs. Most of the book is devoted to the description and analysis of their equilibrium and stability. It is shown that there are measurable characteristics of the proximity of the prominence to the instability threshold, which can be very useful in the problem of space weather forecasting. The book contains many illustrations and links to the latest scientific articles and reviews on the topic. It will be useful to researchers in the field of astrophysics, solar physics, geophysics, as well as PhD and graduate students.
650 0 $a Solar activity. $3 276016
650 1 4 $a Solar Physics. $3 932132
650 2 4 $a Astrophysics. $3 225419
650 2 4 $a Astronomy, Observations and Techniques. $3 376735
650 2 4 $a Astrophysical Plasma. $3 936198
710 2 $a SpringerLink (Online service) $3 273601
773 0 $t Springer Nature eBook
830 0 $a Astrophysics and space science library ; $v 379. $3 557835
856 4 0 $u https://doi.org/10.1007/978-3-031-58177-9
950 $a Physics and Astronomy (SpringerNature-11651)