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Book
Physics of solar prominences : IAU colloquium 44, held in Oslo, August 14-18, 1978
Authors: --- ---
ISBN: 8299055601 Year: 1979 Publisher: Blindern (Oslo) : Institute of Theoretical Astrophysics,

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Keywords

Sun --- Prominences --- Congresses.


Book
Dynamics of quiescent prominences
Authors: ---
ISBN: 354052973X 038752973X Year: 1990 Publisher: Berlin : Springer,

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Book
Nature of prominences and their role in space weather : proceedings of the 300th Symposium of the International Astronomical Union, held in Paris, France, June 10-16, 2013
Authors: --- --- ---
ISBN: 9781107045194 1107045193 Year: 2013 Publisher: Cambridge, United Kingdom Cambridge University Press

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Solar prominences and filaments are large gaseous features extending outward hundreds of thousands of kilometres from the Sun's surface, which play an active role in space weather. Magnetic clouds and interplanetary coronal mass ejections associated with erupting prominences can produce severe perturbations in the Earth's near-space environment. IAU Symposium 300 presents a review of the state-of-the-art theoretical and numerical modelling of prominences and filaments, and their role in the dynamics of Sun-Earth relations. Observations from the latest international space-borne missions (Hinode, STEREO and SDO) and ground-based observatories are presented. The Symposium benefits not just newcomers to solar physics research but it shares the current status of our sophisticated solar analysis with the stellar community, now that huge prominences and CMEs have been detected in solar-type stars, and others, which will affect any exoplanets they host.--Cover page 4.

Keywords

Solar system --- Sun --- Prominences


Book
Plasma loops in the solar corona
Author:
ISBN: 0511600119 Year: 1991 Publisher: Cambridge : Cambridge University Press,

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This book presents the first comprehensive account of the properties of plasma loops, the fundamental structural elements of the solar corona. Plasma loops cover a wide range of sizes, and range in temperature from tens of thousands to millions of degrees. They not only define the structure of individual active regions but connect different active regions - even across the solar equator. Loops also play an integral and decisive role in the enormous solar explosions called flares. Over recent years a wealth of space and ground-based observations of loops has been obtained in various widely-spaced regions of the electromagnetic spectrum. In this book the authors have selected the best observational material from the literature on which to base a detailed account of the properties of flare and non-flare loops. The book also explores the larger implications of the loop structures in our understanding of solar and stellar coronae. The text is enhanced by a large number of illustrations and unique and beautiful photographs obtained from the ground and from space.

Keywords

Sun --- Corona. --- Loop prominences.

Plasma loops in the solar corona
Author:
ISBN: 0521351073 Year: 1991 Volume: 18 Publisher: Cambridge,New York : Cambridge University Press,

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Keywords

Sun --- Loop prominences --- Soleil --- Corona --- Couronne

Dynamics and structure of quiescent solar prominences
Author:
ISBN: 902772833X 9027728348 9400930771 Year: 1989 Volume: vol 150 Publisher: Dordrecht Boston London Kluwer Academic

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Solar prominences
Author:
ISBN: 902770399X 9027704007 9401021368 Year: 1974 Publisher: Dordrecht Reidel

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Book
Solar Prominences
Authors: ---
ISBN: 9783319104164 3319104152 9783319104157 3319104160 Year: 2015 Publisher: Cham : Springer International Publishing : Imprint: Springer,

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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.

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