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Magnetic Coupling Between the Interior and Atmosphere of the Sun

Magnetic Coupling Between the Interior and Atmosphere of the Sun
Author: S. S. Hasan
Publisher:
Total Pages:
Release: 2010
Genre: Solar magnetic fields
ISBN: 9783642028601

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These are the proceedings of the conference on Magnetic Coupling between the Interior and the Atmosphere of the Sun held December 2-5, 2008, which was planned to coincide with the centenary of the discovery of the Evershed effect at Kodaikanal in 1909. The aim of this meeting was to bring a critical focus to the comprehensive understanding of the important issues pertaining to solar magnetism, with particular emphasis on the various MHD processes that operate in the solar atmosphere. The participants reviewed the current status of magnetic field measurements and their implications with regard to recent theories and numerical models that address the fundamental scales and processes in the highly magnetized, turbulent plasma. The conference also provided a platform for in-depth discussions of new results from various space missions, as well as a comparison with ground-based observing facilities such as the Swedish 1-m Solar Telescope.


Magnetic Coupling between the Interior and Atmosphere of the Sun

Magnetic Coupling between the Interior and Atmosphere of the Sun
Author: S.S. Hasan
Publisher: Springer Science & Business Media
Total Pages: 561
Release: 2010-03-10
Genre: Science
ISBN: 3642028594

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Solar physics in India has a tradition that can be traced to the setting up of the Kodaikanal Observatory in 1899 when the Madras Observatory was relocated to a high altitude site with a view to initiate observations of the sun. This conference on Magnetic Coupling between the Interior and the Atmosphere of the Sun during 2–5 December 2008 was planned to coincide with centenary of the Evershed effect discovery at Kodaikanal in 1909. The aim of this meeting was to bring to a critical focus a comprehensive - derstanding of the important issues pertaining to solar magnetism with particular emphasis on the various MHD processes that operate in the solar atmosphere. The current status of magnetic eld measurements and their implications in the light of recenttheoriesandnumericalmodelingthataddressthe fundamentalscalesandp- cessesinthehighlymagnetizedturbulentplasmawerereviewedduringthismeeting. The meeting was timely for the following reasons: Space observations such as from SOHO and TRACE have provided a wealth of multiwavelength observations onprocessesoccurringinregionsofthe atmosphereextendingfromthe photosphere up to the outer corona. With the launch of Hinode and STEREO in 2006 and of SDO (Solar Dynamics Observatory) shortly, this conference provided a platform for in-depth discussions on new results from various space missions as well as a comparison with ground-based observing facilities such as the Swedish 1-m Solar Telescope. Using sophisticated image processing techniques, such telescopes r- tinelygenerateobservationswitharesolutionbetterthan0. 1arcsec,therebyyielding more informative diagnostics for instance of the microstructure of ux tubes.


Magnetohydrodynamics of the Sun

Magnetohydrodynamics of the Sun
Author: Eric Priest
Publisher: Cambridge University Press
Total Pages: 581
Release: 2014-04-07
Genre: Science
ISBN: 0521854717

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This advanced textbook reviews the complex interaction between the Sun's plasma atmosphere and its magnetic field.


Solar Flare Magnetic Fields and Plasmas

Solar Flare Magnetic Fields and Plasmas
Author: Yuhong Fan
Publisher: Springer Science & Business Media
Total Pages: 204
Release: 2012-03-28
Genre: Science
ISBN: 146143761X

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This volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun’s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfer effects into three-dimensional magnetohydrodynamic models of the solar interior and atmosphere, (2) The connection between observed radiation processes occurring during flares and the underlying flare energy release and transport mechanisms, (3) The global balance of forces and momenta that occur during flares, (4) The data-analysis and theoretical tools needed to understand and assimilate vector magnetogram observations and (5) Connecting flare and CME phenomena to the topological properties of the magnetic field in the Solar Atmosphere. The role of the Sun’s magnetic field is a major emphasis of this book, which was inspired by a workshop honoring Richard C. (Dick) Canfield. Dick has been making profound contributions to these areas of research over a long and productive scientific career. Many of the articles in this topical issue were first presented as talks during this workshop and represent substantial original work. The workshop was held 9 – 11 August 2010, at the Center Green campus of the National Center for Atmospheric Research (NCAR) in Boulder, Colorado. This volume is aimed at researchers and graduate students active in solar physics, solar-terrestrial physics and magneto-hydrodynamics. Previously published in Solar Physics journal, Vol. 277/1, 2012.


The Sun-Climate Connection Over the Last Millennium Facts and Questions

The Sun-Climate Connection Over the Last Millennium Facts and Questions
Author: Maxim Ogurtsov
Publisher: Bentham Science Publishers
Total Pages: 252
Release: 2015-01-02
Genre: Science
ISBN: 1608059804

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The search for a cause of the global warming phenomenon on our planet has sparked some interest in the scientific community. The connection between changes occurring in the sun and global warming presents one fundamental perspective which has been investigated by a number of scientific research groups. In recent times, there have been some promising results that might help us uncover the clues about such a link. The Sun-Climate Connection over the Last Millennium: facts and questions presents fundamental information about the solar activity, space weather, terrestrial climates and their variations over an extended period of time. The information presented is a set of analyses based on modern methods of statistical analysis of non-stationary time series, including Fourier, wavelet and singular spectral analysis while considering space weather phenomena (solar winds, solar flares, aurora borealis etc.) and other terrestrial manifestations of solar activity. The physical mechanisms potentially linking solar activity and space weather to climate are discussed based on these analyses. The eBook also provides some context of modern millennial temperature reconstructions for explaining global warming in the 20th century. Scenarios of the solar activity and climate evolution throughout the 21st century are considered on the basis of the updated data. The eBook provides useful facts for researchers seeking information on climate and space research with respect to solar phenomena


Extreme Events in Geospace

Extreme Events in Geospace
Author: Natalia Buzulukova
Publisher: Elsevier
Total Pages: 798
Release: 2017-12-01
Genre: Science
ISBN: 0128127015

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Extreme Events in Geospace: Origins, Predictability, and Consequences helps deepen the understanding, description, and forecasting of the complex and inter-related phenomena of extreme space weather events. Composed of chapters written by representatives from many different institutions and fields of space research, the book offers discussions ranging from definitions and historical knowledge to operational issues and methods of analysis. Given that extremes in ionizing radiation, ionospheric irregularities, and geomagnetically induced currents may have the potential to disrupt our technologies or pose danger to human health, it is increasingly important to synthesize the information available on not only those consequences but also the origins and predictability of such events. Extreme Events in Geospace: Origins, Predictability, and Consequences is a valuable source for providing the latest research for geophysicists and space weather scientists, as well as industries impacted by space weather events, including GNSS satellites and radio communication, power grids, aviation, and human spaceflight. The list of first/second authors includes M. Hapgood, N. Gopalswamy, K.D. Leka, G. Barnes, Yu. Yermolaev, P. Riley, S. Sharma, G. Lakhina, B. Tsurutani, C. Ngwira, A. Pulkkinen, J. Love, P. Bedrosian, N. Buzulukova, M. Sitnov, W. Denig, M. Panasyuk, R. Hajra, D. Ferguson, S. Lai, L. Narici, K. Tobiska, G. Gapirov, A. Mannucci, T. Fuller-Rowell, X. Yue, G. Crowley, R. Redmon, V. Airapetian, D. Boteler, M. MacAlester, S. Worman, D. Neudegg, and M. Ishii. Helps to define extremes in space weather and describes existing methods of analysis Discusses current scientific understanding of these events and outlines future challenges Considers the ways in which space weather may affect daily life Demonstrates deep connections between astrophysics, heliophysics, and space weather applications, including a discussion of extreme space weather events from the past Examines national and space policy issues concerning space weather in Australia, Canada, Japan, the United Kingdom, and the United States


Magnetic Fields in the Solar Atmosphere

Magnetic Fields in the Solar Atmosphere
Author: Jacques Maurice Beckers
Publisher:
Total Pages: 40
Release: 1976
Genre: Magnetohydrodynamics
ISBN:

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This paper describes the magnetic field configurations observed in the solar atmosphere including the corona and the solar wind. The techniques for observing solar magnetic fields are briefly reviewed. The significance of Alfven waves in transporting energy is stressed. (Author).


Solar and Space Physics

Solar and Space Physics
Author: National Research Council
Publisher: National Academies Press
Total Pages: 37
Release: 2014-09-25
Genre: Science
ISBN: 0309313953

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In 2010, NASA and the National Science Foundation asked the National Research Council to assemble a committee of experts to develop an integrated national strategy that would guide agency investments in solar and space physics for the years 2013-2022. That strategy, the result of nearly 2 years of effort by the survey committee, which worked with more than 100 scientists and engineers on eight supporting study panels, is presented in the 2013 publication, Solar and Space Physics: A Science for a Technological Society. This booklet, designed to be accessible to a broader audience of policymakers and the interested public, summarizes the content of that report.


Waves and Oscillations in the Solar Atmosphere (IAU S247)

Waves and Oscillations in the Solar Atmosphere (IAU S247)
Author: International Astronomical Union. Symposium
Publisher: Cambridge University Press
Total Pages: 404
Release: 2008-06-12
Genre: Science
ISBN: 9780521874694

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Provides the latest summary on the solar coronal heating enigma and magneto-seismology of the solar atmosphere, for solar physics researchers.


Solar Prominences

Solar Prominences
Author: Jean-Claude Vial
Publisher: Springer
Total Pages: 490
Release: 2014-11-24
Genre: Science
ISBN: 3319104160

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This volume presents the latest research results on solar prominences, including new developments on e.g. chirality, fine structure, magnetism, diagnostic tools and relevant solar plasma physics. In 1875 solar prominences, as seen out of the solar limb, were described by P.A. Secchi in his book Le Soleil as "gigantic pink or peach-flower coloured flames". The development of spectroscopy, coronagraphy and polarimetry brought tremendous observational advances in the twentieth century. The authors present and discuss exciting new challenges (resulting from observations made by space and ground-based telescopes in the 1990s and the first decade of the 21st century) concerning the diagnostics of prominences, their formation, their life time and their eruption along with their impact in the heliosphere (including the Earth). The book starts with a general introduction of the prominence “object” with some historical background on observations and instrumentation. In the next chapter, the various forms of prominences are described with a thorough attempt of classification. Their thermodynamic (and velocity) properties are then derived with emphasis on the methods (and their limits) used. This goes from the simplest optically thin case to the heavy radiative treatment of plasmas out of local thermodynamic equilibrium. The following chapters are devoted to the magnetic field measurements and indirect derivation. A new branch of diagnostic tools, the seismology, is presented along with some MHD basics. This allows to better understand the propagation of waves, the energy and force equilibria. Both small-scale and large-scale studies and their relationship are presented. The importance of the newly discovered cavities is stressed in the context of prominence destabilization. The issues of prominence formation and eruption, their connection with flares and Coronal Mass Ejections and their impact on the Earth are addressed on the basis of the latest results. Finally, an exciting new area of research is unveiled with the newly discovered evidence of similar manifestations in the Universe and their possible impact on the habitability of exoplanets. References to the basic physics (where necessary) are provided and the proposed web sites addresses will allow the reader to load exciting movies. The book is aimed at advanced students in astrophysics, post-graduates, solar physicists and more generally astrophysicists. Amateurs will enjoy the many new images which go with the text.