9781441922458 - Plasma Astrophysics, Part Ii: Reconnection and Flares: 341 Astrophysics and Space Science Library, 341 by Somov, Boris V (12 results)

Soft cover. Condition: New. Dust Jacket Condition: New. 1st Edition. **INTERNATIONAL EDITION** Read carefully before purchase: This book is the international edition in mint condition with the different ISBN and book cover design, the major content is printed in full English as same as the original North American edition. The book printed in black and white, generally send in twenty-four hours after the order confirmed. All shipments go through via USPS/UPS/DHL with tracking numbers. Great professional textbook selling experience and expedite shipping service.

Trade paperback. Condition: New in new dust jacket. First edition. ***INTERNATIONAL EDITION*** Read carefully before purchase: This book is the international edition in mint condition with the different ISBN and book cover design, the major content is printed in full English as same as the original North American edition. The book printed in black and white, generally send in twenty-four hours after the order confirmed. All shipments contain tracking numbers. Great professional textbook selling experience and expedite shipping service. Trade paperback (US). 440 p. Astrophysics and Space Science Library., 341. Audience: Professional and scholarly.

Condition: New. In.

Condition: New. pp. 440.

Taschenbuch. Condition: Neu. Plasma Astrophysics, Part II | Reconnection and Flares | Boris V. Somov | Taschenbuch | Astrophysics and Space Science Library | Englisch | 2010 | Springer | EAN 9781441922458 | Verantwortliche Person für die EU: Springer Nature Customer Service Center GmbH, Europaplatz 3, 69115 Heidelberg, productsafety[at]springernature[dot]com | Anbieter: preigu.

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Magnetic elds are easily generated in astrophysical plasma owing to its 6 high conductivity. Magnetic elds, having strengths of order few 10 G, correlated on several kiloparsec scales are seen in spiral galaxies. Their origin could be due to ampli cation of a small seed eld by a turbulent galactic dynamo. In several galaxies, like the famous M51, magnetic elds are well correlated (or anti-correlated) with the optical spiral arms. These are the weakest large-scale elds observed in cosmic space. The strongest magnets in space are presumably the so-called magnetars, the highly mag- 15 netized (with the strength of the eld of about 10 G) young neutron stars formed in the supernova explosions. The energy of magnetic elds is accumulated in astrophysical plasma, and the sudden release of this energy - an original electrodynamical 'burst' or'explosion'-takesplaceunderde nitebutquitegeneralconditions(P- att, 1992; Sturrock, 1994; Kivelson and Russell, 1995; Rose, 1998; Priest and Forbes, 2000; Somov, 2000; Kundt, 2001). Such a ' are' in ast- physical plasma is accompanied by fast directed ejections (jets) of plasma, powerful ows of heat and hard electromagnetic radiation as well as by impulsive acceleration of charged particles to high energies.

Paperback. Condition: Brand New. reprint edition. 440 pages. 9.00x6.00x1.04 inches. In Stock.

Condition: new. Questo è un articolo print on demand.

Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This illustrated monograph explores the fundamentals, current practice, and theoretical perspectives of modern plasma astrophysics. The opening part covers basic principles and practical tools for understanding and working with plasma astrophysics. The second section examines the physics of magnetic reconnection and flares of electromagnetic origin in space plasmas in the solar system, and more. Designed mainly for professional researchers, it will be useful to graduate students in space sciences and geophysics. 428 pp. Englisch.

Condition: New. Print on Demand pp. 440 78 Illus. (4 col.).

Condition: New. PRINT ON DEMAND pp. 440.

Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Magnetic elds are easily generated in astrophysical plasma owing to its 6 high conductivity. Magnetic elds, having strengths of order few 10 G, correlated on several kiloparsec scales are seen in spiral galaxies. Their origin could be due to ampli cation of a small seed eld by a turbulent galactic dynamo. In several galaxies, like the famous M51, magnetic elds are well correlated (or anti-correlated) with the optical spiral arms. These are the weakest large-scale elds observed in cosmic space. The strongest magnets in space are presumably the so-called magnetars, the highly mag- 15 netized (with the strength of the eld of about 10 G) young neutron stars formed in the supernova explosions. The energy of magnetic elds is accumulated in astrophysical plasma, and the sudden release of this energy ¿ an original electrodynamical ¿burst¿ or¿explosion¿¿takesplaceunderde nitebutquitegeneralconditions(P- att, 1992; Sturrock, 1994; Kivelson and Russell, 1995; Rose, 1998; Priest and Forbes, 2000; Somov, 2000; Kundt, 2001). Such a ¿ are¿ in ast- physical plasma is accompanied by fast directed ejections (jets) of plasma, powerful ows of heat and hard electromagnetic radiation as well as by impulsive acceleration of charged particles to high energies.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 440 pp. Englisch.