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Geomagnetosphere and Coupling Phenomena: Solar wind

Geomagnetosphere and Coupling Phenomena: Solar wind
Author: Lev Isaakovich Dorman
Publisher:
Total Pages: 0
Release: 2017
Genre: Cosmic rays
ISBN: 9781536105643

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The present review book by Prof., Dr. Lev I. Dorman, Plasmas and Energetic Processes in Geomagnetosphere reflects the development of the geomagnetospheres research and applications for the last few decades. The importance and actuality of geomagnetosphere research are based on the following three factors: 1. The geomagnetosphere is the nearest giant natural laboratory, where it is possible via satellites and ground measurements to investigate in detail many different plasmas and energetic processes in space, which are caused by an interaction of high kinetic energy solar wind plasmas and its perturbations (Interplanetary Coronal Mass Ejections - ICMEs, Interplanetary Shock Waves ISWs, Interplanetary Interaction Regions IIR), including those frozen in the Interplanetary Magnetic Fields (IMF) with the rotated main geomagnetic field. This interaction leads to the dynamic transformation of magnetic fields in the geomagnetosphere, generation and trapping of high energy particles (which are known as Magnetospheric Cosmic Rays MCR), and the generation of many types of instabilities and electromagnetic radiations. These processes are in principle similar to processes in magnetospheres of other planets and their moons, in the atmosphere of the sun and other stars, in interplanetary and in interstellar space, and in many different astrophysical objects. This research is an important basis for fundamental space and astrophysical science. 2. Today, technology, economics, navigation, TV, Internet, radio connections, military aspects, and the life of people on our planet are strongly connected to the work of many satellites moving inside the geomagnetosphere. Different processes and MCR in the geomagnetosphere influence the satellites work and often lead to satellite malfunctions up to fully destroying their electronics; satellites essentially die in these cases. The described research can be considered as a basis for developing methods of forecasting dangerous situations for satellites in different orbits and to decrease the risk of satellite malfunctions and loss. 3. The interaction of ICME, ISW, and IIR with the geomagnetosphere leads to the generation of big magnetic storms accompanied with a Forbush decrease and precursory effects in Galactic Cosmic Ray (GCR) intensity. These magnetic storms are dangerous not only to satellites, but also to the Earths surface in terms of technology, radio connections, car accidents, and human health (e.g., increasing the frequency of infarct myocardial and brain strokes). Investigations of causes of magnetic storms can help to develop methods of forecasting and decreasing the level of magnetic storm hazards. Therefore, the other practical application of this research is connected with the problem of space weather and space climate influence on the technology, radio connections, navigation, transportation, and peoples health on the Earth, which is independent of altitude and geomagnetic latitude.


Geomagnetosphere and Coupling Phenomena: Coupling of the geomagnetosphere

Geomagnetosphere and Coupling Phenomena: Coupling of the geomagnetosphere
Author: Lev I. Dorman
Publisher:
Total Pages: 0
Release: 2017
Genre: Cosmic rays
ISBN: 9781536122701

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This monograph is, as far as the authors have gathered, the first one of its kind which presents various characterisations of many important and continuous distributions. It consists of six chapters. The first chapter lists cumulative distribution functions, probability density functions, hazard functions and reverse hazard functions of one hundred thirty-six important univariate continuous distributions. Chapter Two provides characterisations of these distributions based on the ratio of two truncated moments. Chapter Three takes up the characterisations of some of these distributions in terms of their hazard functions. Chapter Four deals with the characterisations of some of these distributions based on their reverse hazard functions. Characterisations of some of these distributions based on the conditional expectations of certain functions of the random variable are presented in Chapter Five. Finally, to make this book self-contained, we present the characterisations of a large number of distributions (without their proofs) that have already been published by Hamedani and coauthors in Chapter Six.


Magnetosphere-Ionosphere Coupling

Magnetosphere-Ionosphere Coupling
Author: Y. Kamide
Publisher: Springer Science & Business Media
Total Pages: 279
Release: 2012-12-06
Genre: Science
ISBN: 3642500625

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In the past two decades a succession of direct observations by satellites, and of extensive computer simulations, has led to the realization that the polar ionosphere plays a principal role in large-scale magnetospheric processes - a manifestation of the physics linkage involved in solar-terrestrial interactions. Spatial/temporal variations in high-latitude electromagnetic phenomena, such as dynamic aurorae, electric fields and currents, have proved to be extremely complex. Now the challenge is to comprehend the vast amount of complicated measurements made in this magnetosphere-ionosphere sysstem of the Earth. This book addresses the electrical coupling between the hot, but dilute, magnetospheric plasma and the cold, but dense, plasma in the ionosphere. In five major chapters, this book presents: - basic properties of magnetosphere-ionosphere coupling; - morphology of electric fields and currents at high latitudes; - global modeling of magnetosphere-ionosphere coupling; - modeling of ionospheric electrodynamics; - current issues, such as auroral particle acceleration, substorms, penetration of high-latitude fields into low latitudes.


Magnetosphere-Ionosphere Coupling in the Solar System

Magnetosphere-Ionosphere Coupling in the Solar System
Author: Charles R. Chappell
Publisher: John Wiley & Sons
Total Pages: 414
Release: 2016-10-31
Genre: Science
ISBN: 1119066778

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Over a half century of exploration of the Earth’s space environment, it has become evident that the interaction between the ionosphere and the magnetosphere plays a dominant role in the evolution and dynamics of magnetospheric plasmas and fields. Interestingly, it was recently discovered that this same interaction is of fundamental importance at other planets and moons throughout the solar system. Based on papers presented at an interdisciplinary AGU Chapman Conference at Yosemite National Park in February 2014, this volume provides an intellectual and visual journey through our exploration and discovery of the paradigm-changing role that the ionosphere plays in determining the filling and dynamics of Earth and planetary environments. The 2014 Chapman conference marks the 40th anniversary of the initial magnetosphere-ionosphere coupling conference at Yosemite in 1974, and thus gives a four decade perspective of the progress of space science research in understanding these fundamental coupling processes. Digital video links to an online archive containing both the 1974 and 2014 meetings are presented throughout this volume for use as an historical resource by the international heliophysics and planetary science communities. Topics covered in this volume include: Ionosphere as a source of magnetospheric plasma Effects of the low energy ionospheric plasma on the stability and creation of the more energetic plasmas The unified global modeling of the ionosphere and magnetosphere at the Earth and other planets New knowledge of these coupled interactions for heliophysicists and planetary scientists, with a cross-disciplinary approach involving advanced measurement and modeling techniques Magnetosphere-Ionosphere Coupling in the Solar System is a valuable resource for researchers in the fields of space and planetary science, atmospheric science, space physics, astronomy, and geophysics. Read an interview with the editors to find out more: https://eos.org/editors-vox/filling-earths-space-environment-from-the-sun-or-the-earth


Physics Of Geomagnetic Phenomena

Physics Of Geomagnetic Phenomena
Author: S. Matsushita
Publisher: Elsevier
Total Pages: 644
Release: 2013-10-22
Genre: Science
ISBN: 0323141218

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Physics of Geomagnetic Phenomena, Volume I is a comprehensive, balanced, and authoritative introductory text to geomagnetism. The book is divided into three parts encompassing 11 chapters that discuss the advances in geomagnetism, the generation of geomagnetic field phenomena, and the geomagnetic storm generation mechanisms. The first part of the book covers the history, instrumentation, local anomalies, and different types of indices of geomagnetism. The second part discusses the paleomagnetic data for the direction and intensity of the geomagnetic field in ancient times, and then presents an outline of the theoretical interpretations of the main paleomagnetic results. This part also examines earth’s main geomagnetic field and electromagnetic induction. The third part describes the morphologies of solar quiet and lunar daily variations on individual days and on the average, including the methods of obtaining current systems responsible for these variations and their results. Discussions on the geomagnetic variations in the equatorial zone; the neutral atmosphere and the quiet ionosphere; and the various geomagnetic and ionospheric phenomena are also provided.


Cross-Scale Coupling and Energy Transfer in the Magnetosphere-Ionosphere-Thermosphere System

Cross-Scale Coupling and Energy Transfer in the Magnetosphere-Ionosphere-Thermosphere System
Author: Yukitoshi Nishimura
Publisher: Elsevier
Total Pages: 566
Release: 2021-12-07
Genre: Science
ISBN: 0128213736

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Cross-Scale Coupling and Energy Transfer in the Magnetosphere-Ionosphere-Thermosphere System provides a systematic understanding of Magnetosphere-Ionosphere-Thermosphere dynamics. Cross-scale coupling has become increasingly important in the Space Physics community. Although large-scale processes can specify the averaged state of the system reasonably well, they cannot accurately describe localized and rapidly varying structures in space in actual events. Such localized and variable structures can be as intense as the large-scale features. This book covers observations on quantifying coupling and energetics and simulation on evaluating impacts of cross-scale processes. It includes an in-depth review and summary of the current status of multi-scale coupling processes, fundamental physics, and concise illustrations and plots that are usable in tutorial presentations and classrooms. Organized by physical quantities in the system, Cross-Scale Coupling and Energy Transfer in the Magnetosphere-Ionosphere-Thermosphere System reviews recent advances in cross-scale coupling and energy transfer processes, making it an important resource for space physicists and researchers working on the magnetosphere, ionosphere, and thermosphere. Describes frontier science and major science around M-I-T coupling, allowing for foundational understanding of this emerging field in space physics Reviews recent and key findings in the cutting-edge of the science Discusses open questions and pathways for understanding how the field is evolving


The Dynamic Magnetosphere

The Dynamic Magnetosphere
Author: William Liu
Publisher: Springer Science & Business Media
Total Pages: 367
Release: 2011-06-21
Genre: Science
ISBN: 9400705018

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Despite the plethora of monographs published in recent years, few cover recent progress in magnetospheric physics in broad areas of research. While a topical focus is important to in-depth views at a problem, a broad overview of our field is also needed. The volume answers to the latter need. With the collection of articles written by leading scientists, the contributions contained in the book describe latest research results in solar wind-magnetosphere interaction, magnetospheric substorms, magnetosphere-ionosphere coupling, transport phenomena in the plasma sheet, wave and particle dynamics in the ring current and radiation belts, and extra-terrestrial magnetospheric systems. In addition to its breadth and timeliness, the book highlights innovative methods and techniques to study the geospace.


Dayside Magnetosphere Interactions

Dayside Magnetosphere Interactions
Author: Qiugang Zong
Publisher: John Wiley & Sons
Total Pages: 320
Release: 2020-04-07
Genre: Science
ISBN: 1119509637

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Exploring the processes and phenomena of Earth's dayside magnetosphere Energy and momentum transfer, initially taking place at the dayside magnetopause, is responsible for a variety of phenomenon that we can measure on the ground. Data obtained from observations of Earth’s dayside magnetosphere increases our knowledge of the processes by which solar wind mass, momentum, and energy enter the magnetosphere. Dayside Magnetosphere Interactions outlines the physics and processes of dayside magnetospheric phenomena, the role of solar wind in generating ultra-low frequency waves, and solar wind-magnetosphere-ionosphere coupling. Volume highlights include: Phenomena across different temporal and spatial scales Discussions on dayside aurora, plume dynamics, and related dayside reconnection Results from spacecraft observations, ground-based observations, and simulations Discoveries from the Magnetospheric Multiscale Mission and Van Allen Probes era Exploration of foreshock, bow shock, magnetosheath, magnetopause, and cusps Examination of similar processes occurring around other planets The American Geophysical Union promotes discovery in Earth and space science for the benefit of humanity. Its publications disseminate scientific knowledge and provide resources for researchers, students, and professionals. Find out more about this book from this Q&A with the editors


Physics of Geomagnetic Phenomena

Physics of Geomagnetic Phenomena
Author: S. Matsushita
Publisher: Elsevier
Total Pages: 795
Release: 2016-06-03
Genre: Science
ISBN: 1483222527

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Physics of Geomagnetic Phenomena, Volume II covers the advances in geomagnetism and the penetrations into the generation of geomagnetic field phenomena. This book is composed of three chapters and begins with a discussion on various types of phenomenal disturbances, such as ionospheric and geomagnetic disturbance, aurora, and storm. The next chapter describes certain aspects of space geomagnetism based on satellite and rocket observations. This chapter also examines the origins of geomagnetic disturbance phenomena. The last chapter surveys the problems connected with studies of geomagnetic storms and auroras, along with a hydromagnetic model of these phenomena. This book will be of value to physicists, theoreticians, and scientists in allied fields of geomagnetism.