Chromospheric Fine Structure

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Publisher : Springer Science & Business Media
ISBN 13 : 9401021031
Total Pages : 296 pages
Book Rating : 4.36/5 ( download)

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Book Synopsis Chromospheric Fine Structure by : R.G. Athay

Download or read book Chromospheric Fine Structure written by R.G. Athay and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 296 pages. Available in PDF, EPUB and Kindle. Book excerpt: The devotion of an IA U symposium entirely to the topic of chromo spheric fine structure at a time when models of the spherically symmetric chromosphere are still evolving constitutes a valid recognition of the growing feeling among solar astron omers that the chromosphere cannot be understood independently of its discrete structural features. Network structure, which seemingly borders the photospheric supergranule cells, persists intact throughout the chromosphere and most of the chromosphere-corona transition region. The network is the locus of the bright coarse mottles, and the spicule bushes and is the terminus for one end of the quiet chromo spheric fibrils as well. Additionally, it is the locus of most of the magnetic flux of the quiet chromosphere. It is not surprising, therefore, that current studies of the chromosphere tend to center around efforts to better describe the network phenom ena and to ascertain the physical properties of the network features. Clearly, the supergranule cells and associated network structures constitute a fundamental and singularly important feature of solar structure in the boundary layers. Just as it is now clear that much of the chromo spheric fine structure is associated with the network bordering supergranule cells, it seems equally clear that structural features are almost universally associated with both fluid flow and magnetic geometry. Indeed, many observers claim that the brightness features faithfully map the mag netic lines offorce while still others claim that associated with each class of brightness feature there is a more or less unique fluid flow.

Chromospheric Fine Structure

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Author :
Publisher : Springer
ISBN 13 : 9789027702661
Total Pages : 310 pages
Book Rating : 4.67/5 ( download)

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Book Synopsis Chromospheric Fine Structure by : R.G. Athay

Download or read book Chromospheric Fine Structure written by R.G. Athay and published by Springer. This book was released on 1974-11-30 with total page 310 pages. Available in PDF, EPUB and Kindle. Book excerpt: The devotion of an IA U symposium entirely to the topic of chromo spheric fine structure at a time when models of the spherically symmetric chromosphere are still evolving constitutes a valid recognition of the growing feeling among solar astron omers that the chromosphere cannot be understood independently of its discrete structural features. Network structure, which seemingly borders the photospheric supergranule cells, persists intact throughout the chromosphere and most of the chromosphere-corona transition region. The network is the locus of the bright coarse mottles, and the spicule bushes and is the terminus for one end of the quiet chromo spheric fibrils as well. Additionally, it is the locus of most of the magnetic flux of the quiet chromosphere. It is not surprising, therefore, that current studies of the chromosphere tend to center around efforts to better describe the network phenom ena and to ascertain the physical properties of the network features. Clearly, the supergranule cells and associated network structures constitute a fundamental and singularly important feature of solar structure in the boundary layers. Just as it is now clear that much of the chromo spheric fine structure is associated with the network bordering supergranule cells, it seems equally clear that structural features are almost universally associated with both fluid flow and magnetic geometry. Indeed, many observers claim that the brightness features faithfully map the mag netic lines offorce while still others claim that associated with each class of brightness feature there is a more or less unique fluid flow.

Chromospheric Fine Structure

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Author :
Publisher :
ISBN 13 :
Total Pages : 310 pages
Book Rating : 4.77/5 ( download)

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Book Synopsis Chromospheric Fine Structure by : International Astronomical Union. Symposium

Download or read book Chromospheric Fine Structure written by International Astronomical Union. Symposium and published by . This book was released on 1974 with total page 310 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Chromospheric Fine Structure

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Author :
Publisher : Springer
ISBN 13 : 9789027702661
Total Pages : 310 pages
Book Rating : 4.67/5 ( download)

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Book Synopsis Chromospheric Fine Structure by : R.G. Athay

Download or read book Chromospheric Fine Structure written by R.G. Athay and published by Springer. This book was released on 1974-11-30 with total page 310 pages. Available in PDF, EPUB and Kindle. Book excerpt: The devotion of an IA U symposium entirely to the topic of chromo spheric fine structure at a time when models of the spherically symmetric chromosphere are still evolving constitutes a valid recognition of the growing feeling among solar astron omers that the chromosphere cannot be understood independently of its discrete structural features. Network structure, which seemingly borders the photospheric supergranule cells, persists intact throughout the chromosphere and most of the chromosphere-corona transition region. The network is the locus of the bright coarse mottles, and the spicule bushes and is the terminus for one end of the quiet chromo spheric fibrils as well. Additionally, it is the locus of most of the magnetic flux of the quiet chromosphere. It is not surprising, therefore, that current studies of the chromosphere tend to center around efforts to better describe the network phenom ena and to ascertain the physical properties of the network features. Clearly, the supergranule cells and associated network structures constitute a fundamental and singularly important feature of solar structure in the boundary layers. Just as it is now clear that much of the chromo spheric fine structure is associated with the network bordering supergranule cells, it seems equally clear that structural features are almost universally associated with both fluid flow and magnetic geometry. Indeed, many observers claim that the brightness features faithfully map the mag netic lines offorce while still others claim that associated with each class of brightness feature there is a more or less unique fluid flow.

A Study of the Fine Structures in the Solar Chromosphere

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Publisher :
ISBN 13 :
Total Pages : 138 pages
Book Rating : 4.84/5 ( download)

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Book Synopsis A Study of the Fine Structures in the Solar Chromosphere by : Jacques Maurice Beckers

Download or read book A Study of the Fine Structures in the Solar Chromosphere written by Jacques Maurice Beckers and published by . This book was released on 1964 with total page 138 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Fine Structure and Dynamics of the Solar Photosphere (IAU S327)

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Author :
Publisher : Cambridge University Press
ISBN 13 : 9781107170049
Total Pages : 500 pages
Book Rating : 4.44/5 ( download)

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Book Synopsis Fine Structure and Dynamics of the Solar Photosphere (IAU S327) by : Santiago Vargas Domínguez

Download or read book Fine Structure and Dynamics of the Solar Photosphere (IAU S327) written by Santiago Vargas Domínguez and published by Cambridge University Press. This book was released on 2017-10-12 with total page 500 pages. Available in PDF, EPUB and Kindle. Book excerpt: Solar activity has become of increasing importance in our modern society, as many aspects of today's technology could be affected by eruptive phenomena associated with solar magnetic variability. State of the art solar instrumentation is revealing the dynamics of the Sun with unprecedented temporal and spatial resolutions. This volume includes recent results in solar physics research presented at the IAU Symposium 327, the first IAU symposium held in Colombia, in the historical city of Cartagena de Indias, one of the oldest in the Americas. Its main scientific goal was to discuss recent results on the processes shaping the structure of the solar atmosphere and driving plasma eruptions and explosive events in our star. Researchers in both theory and observation, who study structure and activity in the solar atmosphere, discuss a wide range of topics in the field.

A Study of the Fine Structures in the Solar Chromosphere

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Publisher :
ISBN 13 :
Total Pages : 146 pages
Book Rating : 4.49/5 ( download)

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Book Synopsis A Study of the Fine Structures in the Solar Chromosphere by : Jacques Maurice Beckers

Download or read book A Study of the Fine Structures in the Solar Chromosphere written by Jacques Maurice Beckers and published by . This book was released on 1964 with total page 146 pages. Available in PDF, EPUB and Kindle. Book excerpt: "This study of high-resolution solar disk spectroheliograms, or filtergrams, gives one an insight into the horizzontal distribution of chromospheric fine structureswhich is hard to obtain from limb observations. The main part of this paper is concerned with such a study in the light of the Hydrogen H line (6562.8A) and the Calcium K line (3933.7A) ..."--Page iii.

Nuclear Science Abstracts

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Publisher :
ISBN 13 :
Total Pages : 1216 pages
Book Rating : 4.64/5 ( download)

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Book Synopsis Nuclear Science Abstracts by :

Download or read book Nuclear Science Abstracts written by and published by . This book was released on 1976-06 with total page 1216 pages. Available in PDF, EPUB and Kindle. Book excerpt:

The Structure of the Quiet Photosphere and the Low Chromosphere

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Publisher : Springer Science & Business Media
ISBN 13 : 9401034702
Total Pages : 244 pages
Book Rating : 4.08/5 ( download)

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Book Synopsis The Structure of the Quiet Photosphere and the Low Chromosphere by : C. de Jager

Download or read book The Structure of the Quiet Photosphere and the Low Chromosphere written by C. de Jager and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 244 pages. Available in PDF, EPUB and Kindle. Book excerpt: From 17 to 21 April 1967 a Study Week was held in the hotel 'De Bilderberg' near Arnhem, Holland, with the purpose to establish a new, and if possible, generally acceptable working model for the quiet parts of the solar photosphere and low chromosphere. The organizers of the conference hoped that even if this latter goal appeared too far to be reached, such a meeting would still be useful, if only for enumerating the crucial problems in solar photospheric research, and for defining future subjects of research. About twenty solar physicists from outside the Netherlands participated in the Study Week, while some others, though prevented from actively attending, sub mitted their comments before the meeting. The two above-mentioned goals were reached: a working model could be estab lished; yet it became clear that not everyone would agree about this model, and it became obvious too that future research is strongly needed, in particular in the field of line formation (coherence, or non-coherence; local thermal equilibrium), while also the motion field of the photosphere and chromosphere is insufficiently known, and its influence on the formation of spectral lines hardly understood.

Solar Surface Magnetism

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Publisher : Springer Science & Business Media
ISBN 13 : 940111188X
Total Pages : 532 pages
Book Rating : 4.81/5 ( download)

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Book Synopsis Solar Surface Magnetism by : R. J. Rutten

Download or read book Solar Surface Magnetism written by R. J. Rutten and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 532 pages. Available in PDF, EPUB and Kindle. Book excerpt: Observations of the solar magnetic field are largely confined to the radiation emitted from the photosphere, the thin layer of the solar atmosphere which we call "the solar surface". It is from solar surface observations that we must infer the internal structure and the internal magnetohydrodynamic processes that lead to the multitude of fascinat ing phenomena of solar magnetic activity, and from solar surface observations we must also infer the interplay of convection and magnetism that regulates field dispersal, drives the heating of the outer-atmospheric plasma, and generates the solar wind. There is much to be learned from solar surface magnetism in physics and astrophysics; currently, there are rapid developments in this exciting field. The workshop of which this volume contains the proceedings aimed at a synthesis between observers and theorists, both with regard to the discrete elements that are the building blocks of solar magnetism and with regard to the larger-scale spatial and temporal patterns in which the magnetic elements emerge and disappear. The workshop was held during November 1-5, 1993 in Soesterberg, The Netherlands. The fifty participants took a very active part in making the workshop quite a lively one. The articles in these proceedings cover most of the oral and poster presentations, excepting a dozen soon to be published elsewhere.