Heliophysical Processes and Magnetospheric Dynamics

Heliophysical Processes and Magnetospheric Dynamics PDF Author: N. Gopalswamy
Publisher:
ISBN:
Category : Heliosphere (Astrophysics)
Languages : en
Pages : 184

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Book Description

Heliophysical Processes and Magnetospheric Dynamics

Heliophysical Processes and Magnetospheric Dynamics PDF Author: N. Gopalswamy
Publisher:
ISBN:
Category : Heliosphere (Astrophysics)
Languages : en
Pages : 184

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Book Description


Solar Dynamics and its Effects on the Heliosphere and Earth

Solar Dynamics and its Effects on the Heliosphere and Earth PDF Author: Daniel Baker
Publisher: Springer Science & Business Media
ISBN: 038769532X
Category : Science
Languages : en
Pages : 372

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Book Description
This volume helps the reader to understand the ways and means of how dynamical phenomena are generated at the Sun, how they travel through the Heliosphere, and how they affect Earth. It provides an integrated account of the three principal chains of events all the way from the Sun to Earth: the normal solar wind, coronal mass ejections, and solar energetic particles.

The Magnetospheric Cusps: Structure and Dynamics

The Magnetospheric Cusps: Structure and Dynamics PDF Author: Theodore A. Fritz
Publisher: Springer Science & Business Media
ISBN: 1402036051
Category : Science
Languages : en
Pages : 414

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Book Description
This collection of papers will address the question "What is the Magnetospheric Cusp?" and what is its role in the coupling of the solar wind to the magnetosphere as well as its role in the processes of particle transport and energization within the magnetosphere. The cusps have traditionally been described as narrow funnel-shaped regions that provide a focus of the Chapman-Ferraro currents that flow on the magnetopause, a boundary between the cavity dominated by the geomagnetic field (i.e., the magnetosphere) and the external region of the interplanetary medium. Measurements from a number of recent satellite programs have shown that the cusp is not confined to a narrow region near local noon but appears to encompass a large portion of the dayside high-latitude magnetosphere and it appears that the cusp is a major source region for the production of energetic charged particles for the magnetosphere. Audience: This book will be of interest to space science research organizations in governments and industries, the community of Space Physics scientists and university departments of physics, astronomy, space physics, and geophysics.

Heliophysical Processes

Heliophysical Processes PDF Author: Natchimuthuk Gopalswamy
Publisher: Springer
ISBN: 3642113419
Category : Science
Languages : en
Pages : 310

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Book Description
An outgrowth of the first Asia-Pacific Regional School on the International Heliophysical Year (IHY), this volume contains a collection of review articles describing the universal physical processes in the heliospace influenced by solar electromagnetic and mass emissions. The Sun affects the heliosphere in the short term (space weather) and in the long term (space climate) through numerous physical processes that exhibit similarities in various spatial domains of the heliosphere. The articles take into account various aspects of the Sun-heliosphere connection under a systems approach. This volume will serve as a ready reference work for research in the emerging field of heliophysics, which describes the physical processes taking place in the physical space controlled by the Sun out to the local interstellar medium.

Heliophysics

Heliophysics PDF Author:
Publisher:
ISBN:
Category : Government publications
Languages : en
Pages : 166

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Multiscale Processes in the Earth's Magnetosphere: From Interball to Cluster

Multiscale Processes in the Earth's Magnetosphere: From Interball to Cluster PDF Author: Jean-Andre Sauvaud
Publisher: Springer Science & Business Media
ISBN: 9781402027666
Category : Science
Languages : en
Pages : 356

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Book Description
The past forty years of space research have seen a substantial improvement in our understanding of the Earth’s magnetosphere and its coupling with the solar wind and interplanetary magnetic ?eld (IMF). The magnetospheric str- ture has been mapped and major processes determining this structure have been de?ned. However, the picture obtained is too often static. We know how the magnetosphere forms via the interaction of the solar wind and IMF with the Earth’s magnetic ?eld. We can describe the steady state for various upstream conditions but do not really understand the dynamic processes leading from one state to another. The main dif?culty is that the magnetosphere is a comp- cated system with many time constants ranging from fractions of a second to days and the system rarely attains a steady state. Two decades ago, it became clear that further progress would require multi-point measurements. Since then, two multi-spacecraft missions have been launched — INTERBALL in 1995/96 and CLUSTER II in 2000. The objectives of these missions d- fered but were complementary: While CLUSTER is adapted to meso-scale processes, INTERBALL observed larger spatial and temporal scales. However, the number of papers taking advantage of both missions simul- neously is rather small.

Improving the Understanding of Kinetic Processes in Solar Wind and Magnetosphere: From CLUSTER to MMS

Improving the Understanding of Kinetic Processes in Solar Wind and Magnetosphere: From CLUSTER to MMS PDF Author: Antonella Greco
Publisher: Frontiers Media SA
ISBN: 2889662411
Category : Science
Languages : en
Pages : 137

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Book Description


Quantitative Aspects of Magnetospheric Physics

Quantitative Aspects of Magnetospheric Physics PDF Author: Larry R. Lyons
Publisher: Springer Science & Business Media
ISBN: 9789027716637
Category : Science
Languages : en
Pages : 246

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Book Description
The discovery of the earth's radiation belts in 1957 marked the beginning of what is now known as magnetospheric physics. The field has evolved normally from an early discovery phase through a period of exploration and into an era of quantitative studies of the dynamics of magnetized plasmas as they occur in nature. Such environments are common throughout the universe and have been studied in varying detail at the sun, the planets, pulsars, and certain radio galaxies. The purpose of this book is to describe basic quantitative aspects of magnetospheric physics. We use selected examples from the earth's magnetosphere to show how theory and data together form a quantitative framework for magnetospheric research. We have tried to organize the material along the philosophy of starting simply and adding com plexity only as necessary. We have avoided controversial and relatively new research topics and have tried to use as examples physical processes generally accepted as important within the earth's magnetospheric system. However, even in some of our examples, the question of whether the physical process applied to a particular problem is the dominant process, has yet to be answered.

Heliophysics: Plasma Physics of the Local Cosmos

Heliophysics: Plasma Physics of the Local Cosmos PDF Author: Carolus J. Schrijver
Publisher: Cambridge University Press
ISBN: 1107392705
Category : Science
Languages : en
Pages :

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Book Description
Heliophysics is a developing scientific discipline integrating studies of the Sun's variability, the surrounding heliosphere, and climatic environments. Over the past few centuries, our understanding of how the Sun drives space weather and climate on the Earth and other planets has advanced at an ever-increasing rate. This volume, the first in this series of three heliophysics texts, integrates such diverse topics for the first time as a coherent intellectual discipline. It emphasises the physical processes coupling the Sun and Earth, allowing insights into the interaction of the solar wind and radiation with the Earth's magnetic field, atmosphere and climate system. It provides a core resource for advanced undergraduates and graduates, and also constitutes a foundational reference for researchers in heliophysics, astrophysics, plasma physics, space physics, solar physics, aeronomy, space weather, planetary science and climate science. Additional online resources, including lecture presentations and other teaching materials, are accessible at www.cambridge.org/9780521110617.

Alfvén Waves Across Heliophysics

Alfvén Waves Across Heliophysics PDF Author: Andreas Keiling
Publisher: John Wiley & Sons
ISBN: 1394195966
Category : Science
Languages : en
Pages : 325

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Book Description
Alfvén Waves Across Heliophysics Progress, Challenges, and Opportunities Alfvén waves are fundamental to the dynamics of space plasmas. Recent advances in our knowledge about Alfvén waves have come from several directions, including new space missions to unexplored heliospheric regions, sophisticated rocket campaigns in the auroral zone, enlarged magnetometer arrays and radar networks, and significant advances in computer modeling. Alfvén Waves Across Heliophysics: Progress, Challenges, and Opportunities is an interdisciplinary collaboration from different space science communities to review recent and current Alfvén wave research. Volume highlights include: Alfvén waves in the solar atmosphere Alfvén waves at the giant planets Alfvén waves at Mars Alfvén waves in moon-magnetosphere systems Alfvén waves in geospace Alfvén waves in the laboratory 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.