Eruptions on the Sun

Filippov, Boris

Eruptions on the Sun
  • 出版商: Springer
  • 出版日期: 2024-06-29
  • 售價: $6,860
  • 貴賓價: 9.5 折 $6,517
  • 語言: 英文
  • 頁數: 395
  • 裝訂: Hardcover - also called cloth, retail trade, or trade
  • ISBN: 3031581768
  • ISBN-13: 9783031581762

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相關主題

商品描述

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 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.

商品描述(中文翻譯)

本書專注於太陽上的爆發現象，這是太空天氣干擾最危險的來源。它討論了這一領域的最新成就，這些成就在科學文獻中有所描述，並由作者本人獲得。本書的前幾章簡要描述了太陽在人類生活和歷史中的作用，太陽內部和太陽大氣層的一般描述，太陽活動的原因和驅動因素以及其對地球環境和人類生活的影響。本書詳細描述了太陽上的爆發現象，回顧了太陽活動的觀測和關於太陽大氣層中能量突然釋放的機制和原因的理論觀點。

本書非常關注太陽磁場，它們在光球中的特徵和測量值，在色球和日冕中觀察到的表現，以及將光球數據外推到太陽大氣層上層的方法。假設磁場是在爆發現象中突然釋放的能量的來源，這些現象以耀斑、日珥爆發和日冕物質抛射（CME）的形式觀察到。能量在日冕磁場的非電位（與電流相關）部分中積累和儲存（自由磁能）。這部分磁場是最變化的，可以為快速爆發過程提供能量。CME在星際介質中傳播時，會對其產生顯著的干擾，並在影響地球磁層時引發最強烈的地磁風暴。預測CME到達的時間是整個太空天氣預報的關鍵問題。因此，CME源區的爆發前條件非常重要。太陽日珥和日冕結構被認為是CME最有可能的前體。

本書的大部分內容都是關於太陽日珥和日冕結構的描述和分析。書中展示了接近不穩定閾值的日珥的可測量特徵，這對於太空天氣預報問題非常有用。本書包含許多插圖和鏈接到最新的科學文章和評論。它將對天體物理學、太陽物理學、地球物理學的研究人員以及博士和研究生學生非常有用。

作者簡介

Boris Filippov graduated from Moscow Lomonosov State Univerity (Physical departament) in 1975. He then joined the staff of the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Academy of Sciences of the USSR (IZMIRAN) in 1975. He received received his Ph. D. (Physics and Mathematics) from Pulkovo Observatory in 1984 and Doctor of Sciences (Physics and Mathematics) from IZMIRAN in 1998. From 2017 he has been a Chief Researcher of the Deparment of Solar Physics and Solar-Terrrestrial Relations.

Boris Filippov published more than 150 referred papers in scientific journals, several books: "The Magnetic Fields of Solar Active Regions " (Moscow: Nauka,1992, in co-authorship with M.M. Molodensky, in Russian), "Eruptive Processes on the Sun" (Moscow: Fizmatlit, 2007, in Russian), "Cosmic Environment Around Us" (Troitsk: Trovant, 2006, in co-authorship), and chapters in collective books: "Solar Physics Research Trends", Chapter 1 (Edited by Pingzhi Wang, New York: Nova Science Publishers, Inc., 2008), "Exploring the Solar Wind", Chapter 12, in co-authorship with A.G. Tlatov (Edited by Marian Lazar, Rijeka, Croatia: InTech, 2012), "Horizons in Earth Science Research", Volume 7, Chapter 2 (Edited by Benjamin Veress and Jozsi Szigethy, New York: Nova Science Publishers, Inc., 2012).

作者簡介(中文翻譯)

鮑里斯·菲利波夫於1975年畢業於莫斯科羅蒙諾索夫國立大學物理系。同年，他加入了蘇聯科學院普什科夫地球磁場、電離層和無線電波傳播研究所（IZMIRAN）的工作人員。他於1984年在普爾科沃天文台獲得物理和數學博士學位，並於1998年在IZMIRAN獲得物理和數學博士學位。自2017年以來，他一直擔任太陽物理和太陽地球關係部門的首席研究員。

鮑里斯·菲利波夫在科學期刊上發表了150多篇被引用的論文，並出版了幾本書籍，包括《太陽活躍區的磁場》（莫斯科：Nauka，1992年，與M.M. Molodensky合著，俄文）、《太陽爆發過程》（莫斯科：Fizmatlit，2007年，俄文）、《我們周圍的宇宙環境》（特羅伊茨克：Trovant，2006年，與他人合著），以及在集體著作中的章節，包括《太陽物理研究趨勢》第1章（編輯：Pingzhi Wang，紐約：Nova Science Publishers，Inc.，2008年）、《探索太陽風》第12章，與A.G. Tlatov合著（編輯：Marian Lazar，克羅地亞里耶卡：InTech，2012年）、《地球科學研究的視野》第7卷第2章（編輯：Benjamin Veress和Jozsi Szigethy，紐約：Nova Science Publishers，Inc.，2012年）。

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