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020 _a9783031581779
_9978-3-031-58177-9
024 7 _a10.1007/978-3-031-58177-9
_2doi
050 4 _aQB520-545
072 7 _aPGS
_2bicssc
072 7 _aSCI004000
_2bisacsh
072 7 _aPGS
_2thema
100 1 _aFilippov, Boris.
_eauthor.
_4aut
_4http://id.loc.gov/vocabulary/relators/aut
_979608
245 1 0 _aEruptions on the Sun
_h[electronic resource] /
_cby Boris Filippov.
250 _a1st ed. 2024.
264 1 _aCham :
_bSpringer Nature Switzerland :
_bImprint: Springer,
_c2024.
300 _aX, 393 p. 226 illus., 152 illus. in color.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aAstrophysics and Space Science Library,
_x2214-7985 ;
_v471
505 0 _aIntroduction -- 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 _aThis 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 _aSun.
_968136
650 0 _aAstrophysics.
_968037
650 0 _aAstronomy
_xObservations.
_967976
650 0 _aPlasma astrophysics.
_973287
650 1 4 _aSolar Physics.
_968138
650 2 4 _aAstrophysics.
_968037
650 2 4 _aAstronomy, Observations and Techniques.
_967977
650 2 4 _aAstrophysical Plasma.
_973288
710 2 _aSpringerLink (Online service)
773 0 _tSpringer Nature eBook
776 0 8 _iPrinted edition:
_z9783031581762
776 0 8 _iPrinted edition:
_z9783031581786
776 0 8 _iPrinted edition:
_z9783031581793
830 0 _aAstrophysics and Space Science Library,
_x2214-7985 ;
_v471
_973290
856 4 0 _uhttps://doi.org/10.1007/978-3-031-58177-9
912 _aZDB-2-PHA
912 _aZDB-2-SXP
999 _c61148
_d61148