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Titlebook: Eruptions on the Sun; Boris Filippov Book 2024 The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature

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書目名稱Eruptions on the Sun
編輯Boris Filippov
視頻videohttp://file.papertrans.cn/321/320715/320715.mp4
概述Provides a comprehensive review of solar eruptive phenomena.Discusses solar observations in tandem with the relevant physics.Offers possible ways for a more reliable forecast of space weather
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Eruptions on the Sun;  Boris Filippov Book 2024 The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature
描述.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 c
出版日期Book 2024
關鍵詞Coronal Mass Ejections; Solar Flares; Prominences; Solar Eruptive Events; Space Weather
版次1
doihttps://doi.org/10.1007/978-3-031-58177-9
isbn_softcover978-3-031-58179-3
isbn_ebook978-3-031-58177-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl
The information of publication is updating

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https://doi.org/10.1007/978-3-642-76344-1cribed. More attention is paid to the solar atmosphere, where solar activity phenomena are rape and developed. Some instruments for observations of the Sun, especially the upper layers of the solar atmosphere, which are impossible from the ground level, are listed, as well as space missions dedicate
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https://doi.org/10.1057/9781137360823itting of spectral lines in the early twentieth century. After the invention of the photoelectric solar magnetograph in the mid-twentieth century, it became clear that magnetic fields are present almost everywhere in the photosphere, but they are distributed very unevenly. The strongest fields are o
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https://doi.org/10.1007/978-3-642-92045-5ial equilibrium of prominences, different parameters must be achieved for an eruption to begin. In sheared arcade models, there should be a significant increase in shear. In flux-rope models, there is a critical value of twist at which kink instability occurs. The catastrophic loss of equilibrium an
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