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Book Stellar Winds and Related Flows

Download or read book Stellar Winds and Related Flows written by Thomas Edward Holzer and published by . This book was released on 1970 with total page 666 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Stellar Winds and Related Flows

Download or read book Stellar Winds and Related Flows written by Thomas Edward Holzer and published by . This book was released on 1970 with total page 616 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Introduction to Stellar Winds

    Book Details:
  • Author : Henny J. G. L. M. Lamers
  • Publisher : Cambridge University Press
  • Release : 1999-06-17
  • ISBN : 9780521595650
  • Pages : 456 pages

Download or read book Introduction to Stellar Winds written by Henny J. G. L. M. Lamers and published by Cambridge University Press. This book was released on 1999-06-17 with total page 456 pages. Available in PDF, EPUB and Kindle. Book excerpt: The first comprehensive introduction to the observations and theories of stellar winds; a long-awaited graduate textbook, written by two founders of the field.

Book Hydrodynamics and Stellar Winds

Download or read book Hydrodynamics and Stellar Winds written by Walter J. Maciel and published by Springer Science & Business Media. This book was released on 2014-02-11 with total page 191 pages. Available in PDF, EPUB and Kindle. Book excerpt: Introduces hydrodynamics to undergraduate students in physics and astrophysics. Stellar winds are a common phenomenon in the life of stars, from the dwarfs like the Sun to the red giants and hot supergiants, constituting one of the basic aspects of modern astrophysics. Stellar winds are a hydrodynamic phenomenon in which circumstellar gases expand towards the interstellar medium. This book presents an elementary introduction to the fundamentals of hydrodynamics with an application to the study of stellar winds. The principles of hydrodynamics have many other applications, so that the book can be used as an introduction to hydrodynamics for students of physics, astrophysics and other related areas.

Book Introduction to Stellar Winds

    Book Details:
  • Author : Henny J. G. L. M. Lamers
  • Publisher : Cambridge University Press
  • Release : 1999-06-17
  • ISBN : 9780521593984
  • Pages : 454 pages

Download or read book Introduction to Stellar Winds written by Henny J. G. L. M. Lamers and published by Cambridge University Press. This book was released on 1999-06-17 with total page 454 pages. Available in PDF, EPUB and Kindle. Book excerpt: This long-awaited graduate textbook, written by two pioneers in the field, provides a comprehensive introduction to the observations, theories, and consequences of stellar winds. The rates of mass loss and the wind velocities are explained from basic physical principles. This textbook also includes chapters clearly explaining the formation and evolution of interstellar bubbles and the effects of mass loss on the evolution of high- and low-mass stars. Each topic is introduced simply to explain the basic processes and then developed to provide a solid foundation for understanding current research. This authoritative textbook is designed for advanced undergraduate and graduate students and researchers seeking an understanding of stellar winds and, more generally, supersonic flows from astrophysical objects. It is based on courses taught in Europe and the United States over the past twenty years and includes seventy problems for coursework or self-study.

Book Solar Wind

    Book Details:
  • Author : Charles P. Sonett
  • Publisher :
  • Release : 1972
  • ISBN :
  • Pages : 744 pages

Download or read book Solar Wind written by Charles P. Sonett and published by . This book was released on 1972 with total page 744 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Cosmic Winds and the Heliosphere

Download or read book Cosmic Winds and the Heliosphere written by Jack Randolph Jokipii and published by University of Arizona Press. This book was released on 1997-10 with total page 1060 pages. Available in PDF, EPUB and Kindle. Book excerpt: Contributors examine the physics of wind origin and physical phenomena in winds, including heliospheric shocks, magnetohydrodynamic turbulence, and kinetic phenomena--and their interactions with surrounding media. Contributions range from studies of the interstellar cloud surrounding the solar system to solar wind interaction with comets.

Book Two dimensional Models of Stellar Wind Bubbles

Download or read book Two dimensional Models of Stellar Wind Bubbles written by Michal Różyczka and published by . This book was released on 1984 with total page 25 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book NASA SP

    Book Details:
  • Author :
  • Publisher :
  • Release : 1962
  • ISBN :
  • Pages : 740 pages

Download or read book NASA SP written by and published by . This book was released on 1962 with total page 740 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book The Stellar Wind Regions

Download or read book The Stellar Wind Regions written by Eugene Newman Parker and published by . This book was released on 1960 with total page 1 pages. Available in PDF, EPUB and Kindle. Book excerpt: WITH CLASS G main sequence and M-giant stars are given for various interst llar environments. The supersonic wind from a class G star undergoes a shock transition to subsonic flow at a radial distance of 100 - 1,000 a.u. and may extend many times farther as a subsonic flow. Thic storms. Open-ended Terms: Stellar Wind. From the observations of the solar wind and of the M-giant alpha-Herculis the gross dynamical features of the stellar wind region associated with class G main sequence and M-giant stars are given for various interst llar environments. The supersonic wind from a class G star undergoes a shock transition to subsonic flow at a radial distance of 100 - 1,000 a.u. and may extend many times farther as a subsonic flow. This subsonic flow will be subject to turbulence and oth r instabilities in many cases. The wind from an Mgiant may extend many parsecs if the M-giant p ase of evolution lasts long enough for its wind to approach equilibrium; the resultant in erstellar contamination and heating is important for a distance of many parsecs. A rough calculation of the cavity formed by a stellar wind in a largescale interstellar field is carried out, and it is found that the cavity shape and dimensions for stationary flow depend upon the back pressure at infinity. As the pressure increases, the cavity changes from a circular cylinder of infinite radius, through an increa ingly bulbous shape of finite radius, to a sphere of infinite radius with one finite cyli drical channel from each pole. (Author).

Book Physics of Space  Growth Points and Problems

Download or read book Physics of Space Growth Points and Problems written by Nicole Meyer-Vernet and published by Springer Science & Business Media. This book was released on 2001-11-30 with total page 414 pages. Available in PDF, EPUB and Kindle. Book excerpt: This book contains the Proceedings of the second "Rencontres de l'Observatoire" devoted to Physics of Space: Growth Points and Problems, held at the Paris Observatory at Meudon, on January 10-14, 2000. The last quarter of the century has seen the vertiginous growth of space achievements and the exploration of much of the heliosphere with beautifully instrumented space probes. Even though the heliosphere is merely one particular cosmic environment, it is presently the only one accessible to in situ measurements and hence plays a unique role as a natural laboratory for physics and astrophysics. In this spirit, the conference highlighted recent achievements which have changed our view of the physics of space, with emphasis on the bridges between space plasma physics and other disciplines. The contributions include the physics of collisionless plasmas - in particular particle acceleration and dissipation, dusty plasmas, cosmic winds and jets, the environments of planetary bodies and pulsars, novel space detection techniques, and some landmarks of space physics history and possible futures.

Book Energy Research Abstracts

Download or read book Energy Research Abstracts written by and published by . This book was released on 1985 with total page 792 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Nuclear Science Abstracts

Download or read book Nuclear Science Abstracts written by and published by . This book was released on 1971 with total page 1378 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Cyclical Variability in Stellar Winds

Download or read book Cyclical Variability in Stellar Winds written by Lex Kaper and published by Springer Science & Business Media. This book was released on 2013-06-05 with total page 426 pages. Available in PDF, EPUB and Kindle. Book excerpt: It is well known that stellar winds are variable, and the fluctuations are often cyclical in nature. This property seems to be shared by the winds of cool and hot stars, even though their outflows are driven by fundamentally different physical mechanisms. Since very similar models have been proposed to explain the cyclical wind variations observed in a wide variety of stars, the time was ripe for astrophysicists from many different sub-disciplines to present the state of the art in a concise form. The proceedings will provide a useful, up-to-date overview of the observations, interpretation, and modelling of the time-dependent mass outflows from all sorts of stars.

Book Solar and Astrophysical Magnetohydrodynamic Flows

Download or read book Solar and Astrophysical Magnetohydrodynamic Flows written by Kanaris Tsinganos and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 770 pages. Available in PDF, EPUB and Kindle. Book excerpt: Modern observations, including recent ones with the Hubble Space Telescope, have revealed that the Universe is replete with plasma outflows from all kinds of objects, ranging from stars in all their variety to galaxies. In this masterly survey of plasma astrophysics, written by leading practitioners, the first 15 articles in Part I deal with the use of the MHD approach in several key problems of solar plasma, such as magnetoconvection and magnetic field generation, sunspots and coronal loops, magnetic nonequilibrium and coronal heating, coronal mass ejections, the acceleration of the solar wind, and stellar winds across the Main Sequence. The following 16 articles of Part II deal with the use of the same MHD approach in several central and puzzling aspects of more distant astrophysical plasmas, such as the dynamics of the interstellar medium, collimated outflows from young stellar objects and accretion disks, molecular outflows and jets associated with enigmatic binaries and symbiotic stars, relativistic flows associated with superluminal microquasars in our own galaxy, astrophysical jets from nearby galaxies, or remote active galactic nuclei and quasars, probably fuelled by supermassive black holes. The emphasis throughout is on the striking underlying similarities in the physics of all these problems. Audience: Indispensable for solar physicists and astrophysics alike. An ideal textbook for graduate students in physics and astrophysics.

Book Research in Progress

Download or read book Research in Progress written by and published by . This book was released on 1973 with total page 494 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Magnetosphere and Solar Winds  Humans and Communication

Download or read book Magnetosphere and Solar Winds Humans and Communication written by Khalid S. Essa and published by BoD – Books on Demand. This book was released on 2022-10-05 with total page 224 pages. Available in PDF, EPUB and Kindle. Book excerpt: Magnetosphere and Solar Winds, Humans and Communication consists of ten chapters organized into two sections. The first section presents a full description of the magnetosphere and its effect on the solar wind, climatic modes, the Polar Cap index in relation to magnetosphere disturbances (substorms and magnetic storms), recent developments and challenges in developed ionosphere models, and more. The second section discusses solar flux, solar proton activity over the solar cycle, temporal variation of the sun’s activity, and macroscopic scales of spin.