Magnetotail physics



Publisher: Johns Hopkins University Press in Baltimore

Written in English
Published: Pages: 433 Downloads: 436
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Subjects:

  • Magnetotails -- Congresses.

Edition Notes

Statementedited by Anthony T.Y. Lui.
SeriesJohns Hopkins studies in Earth and planetary sciences
ContributionsLui, Anthony T. Y., Chapman, Sydney, 1888-1970., American Geophysical Union., Chapman Conference on Magnetophysics (1985 : Johns Hopkins University Applied Physics Laboratory)
Classifications
LC ClassificationsQC809.M35 M335 1987
The Physical Object
Paginationxiv, 433 p. :
Number of Pages433
ID Numbers
Open LibraryOL2733379M
ISBN 100801834961
LC Control Number86027614

Other Important Magnetotail Phenomena.- Brief Appearance of Energetic Electrons in the Plasma Sheet.- Leakage of Plasma Sheet Particles into the Magnetosheath.- Preface / A. Nishida, D.N. Baker and S.W.H. Cowley --The Distant Magnetotail: Its Structure, IMF Dependence, and Thermal Properties / K. Maezawa and T. Hori --Large-Scale Structure of the Magnetosphere / D.N. Baker and T.I. Pulkkinen --The Low-Latitude Boundary Layer in the Tail-Flanks / M. Fujimoto, T. Terasawa and T. Mukai --Cold Dense Ion.   Comparing the temperature increase observed in this magnetotail jet to magnetopause and solar wind reconnection jets, we find that the value ± (in terms of the fraction of energy released) is larger than the average of ∼ reported in these other regions [Phan et al., ; Drake et al., ]. However, it is unclear whether this. This COSPAR Colloquium Series deals with the main achievements that were accomplished through the collaborative efforts among ISTP participants; the plasma dynamics of magnetic reconnection in a thin plasma sheet, the action of the solar wind on the plasma population in the plasma sheet and around the magnetotail boundary layer, the relationship between the substrom expansion region and the X.

Current sheets with strong transverse (cross field) currents are commonly observed in planetary magnetospheres and serve as a natural energy source for magnetic reconnection. As . Find many great new & used options and get the best deals for Magnetospheric Multiscale: A Mission to Investigate the Physics of Magnetic Reconnection (, Hardcover) at the best online prices at eBay! Free shipping for many products! Akasofu SI. () Magnetotail Phenomena during Magnetospheric Substorms. In: Physics of Magnetospheric Substorms. Astrophysics and Space Science Library (A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews), vol Springer. For a given flow, there exists a critical value of R m, at which the growth rate of the magnetic field perturbation is the R m increases further, the growth rate of the large-scale magnetic fields decreases to zero, implying that a finite magnetic diffusivity (finite conductivity) of the fluid is necessary for dynamo action. This type of dynamo is often called a slow dynamo, to.

Electromagnetism (Dover Books on Physics) John C. Slater. out of 5 stars Paperback. $ # Electrodynamics: The Field-Free Approach: Electrostatics, Magnetism, Induction, Relativity and Field Theory (Undergraduate Lecture Notes in Physics) Kjell Prytz. On the intersection between space physics and plasma astrophysics, see also the chapter titled “Connections Between Solar and Space Physics and Other Disciplines” in the recent NRC report The Sun to the Earth—and Beyond: A Decadal Research Strategy in Solar and Space Physics, The National Academies Press, Washington, D.C.,   Book Search tips Selecting this option will search all publications across the Scitation platform Magnetic reconnection is one of the key processes inherent to plasma physics, responsible for the topological and R. Nakamura, “ Magnetotail reconnection,” in Magnetic Reconnection: Concepts and Applications, Astrophysics. March Geotail Book Awarded by Publishing Industry. The monograph New Perspectives on the Earth's Magnetotail has been selected by the Association of American Publishers as the best professional and scholarly book in physics and astronomy for New Perspectives was edited by Atsuhiro Nishida, director-general of ISAS and project scientist for the Geotail mission; Daniel N. .

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Magnetotail Physics (Johns Hopkins Studies in Earth and Planetary Sciences) by Professor Anthony T.Y. Lui (Editor) ISBN ISBN Why is ISBN important. ISBN. This bar-code number lets you verify that you're getting exactly the right version or edition of a book.

The digit and digit formats both work. COVID Resources. Reliable information about the coronavirus (COVID) is Magnetotail physics book from the World Health Organization (current situation, international travel).Numerous and frequently-updated resource results are available from this ’s WebJunction has pulled together information and resources to assist library staff as they consider how to handle coronavirus.

The monograph Magnetotail Physics, edited by An­ thony T. Lui, is a welcome and long-awaited relief. It is based on review papers and contributed papers D. Papadopoulos is a professor in the Department of Physics.

Recent theoretical and experimental investigations of magnetotails (MTs) are examined in reviews and reports based on papers presented at the Chapman Conference on Magnetotail Physics, held at the Johns Hopkins University Applied Physics Laboratory in October All aspects of space plasmas in the Solar System are introduced and explored in this text for senior undergraduate and graduate students.

Introduction to Space Physics provides a broad, yet selective, treatment of the complex interactions of the ionized gases of the solar terrestrial environment. The book includes extensive discussion of the Sun and solar wind, the magnetized and unmagnetized 5/5(3).

The book, New Perspectives on the Earth's Magnetotail, records the great achievements in magnetotail physics over the past book was judged on both its scientific merits and relevance to award-winning volume, which drew much from the new information obtained by the GEOTAIL mission, provides first-hand information Magnetotail physics book the generation mechanisms for energetic particles.

The author discusses observed kinetic (as opposed to fluid) aspects of particle behavior in the geomagnetic tail. Such behavior has been observed from thermal plasma energies to energies greater than or approximately equal to a few MeV.

By presenting examples of observed kinetic effects throughout the energy range observed in the tail, the author demonstrates the importance of recognizing and.

About this book All magnetized planets in our solar system (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) interact strongly with the solar wind and possess well developed magnetotails.

It is not only the strongly magnetized planets that have magnetotails. We compare the results of fully kinetic simulations with observed electron velocity distributions in a magnetotail reconnection diffusion region and use the maximum entropy model to reconstruct electron and ion distributions using various numbers of moments obtained from the.

Abstract We present a statistical analysis of more than electrostatic solitary waves interpreted as electron holes (EH) measured aboard at least three MMS spacecraft in the Earth's magnetotail.

A new study by Zhong et al. () uses high‐resolution Magnetospheric Multiscale Mission (MMS) measurements of a flux rope in the Earth's magnetotail in order to identify the accelerationmechanisms at play and link them to “smoking gun” signatures in.

A definition is introduced that is applicable to the two generic classes of magnetotails that are now recognized. The earth's magnetotail is the most extensively surveyed of all magnetotails and is used as a prototype to illustrate the various magnetotail plasma domains.

Typical values and variations of magnetotail parameters are discussed briefly. The flapping motion of Mercury's magnetotail current sheet is investigated based on the observations of MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER).

The typical flapping period in Mercury's magnetotail is much shorter (~13 s), comparing with ~10–20 min at Earth's magnetotail. adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A.

In the Earth's magnetotail, plasmoids can be considered as a particular type of large-scale island that form between a near-Earth X-line and the last closed plasma sheet field line, whose farthest downtail point is notionally referred to as the distant X-line (e.g., Hones ; Slavin et al.

; Baker et al. The Earth's magnetotail plays an important role in the solar-wind–magnetosphere coupling. At the midplane of the magnetotail is a current sheet where the dominant magnetic field component reverses. A magnetosphere is a region of space surrounding an astronomical object in which charged particles are affected by that object's magnetic field.

It is created by a star or planet with an active interior dynamo. In the space environment close to a planetary body, the magnetic field resembles a magnetic r out, field lines can be significantly distorted by the flow of electrically.

Recent in-situ spacecraft observations in the dipolarized magnetotail (i.e., observations behind the dipolarization front in the quiet magnetotail plasma sheet) have revealed the abundance of sub-ion scale (~ km size) magnetic holes (Ge et al., ; Ji et al., ; Gershman et al., ).

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It too is being actively rewritten and developed, no guarantees, but it is probably still useful in its current incarnation. Fiction • The Book of Lilith ISBN: Sonnerup, in Solar System Plasma Physics, vol. III, L. Lanzerotti, C. Kennel, E.

Parker, eds., North-Holland, New York (), p. According to this picture, reconnection begins when the solar wind squeezes a part of the magnetotail from above and below the so-called X-line, the notional locus of a reconnection event (see figure. Physics of Magnetospheric Substorms.

[Syun-Ichi Akasofu] -- Man, through intensive observations of natural phenomena, has learned about some of the basic principles which govern nature. Geomagnetic and Magnetospheric Storms --References Magnetotail Phenomena During Magnetospheric Substorms A Series of Books on the Recent.

Purchase Frontiers in Magnetospheric Plasma Physics, Volume 16 - 1st Edition. Print Book & E-Book. ISBN  These particles, plus many more mantle particles, then propagate tailward on open (lobe like) field lines. In the magnetotail many of the particles encounter and enter the flux rope region.

Particles affected by magnetic reconnection in the magnetotail associated with the flux rope can increase their energy by several keV. A discussion of why a magnetotail is a fundamental issue in magnetospheric physics A unique collection of tutorials that cover a large range of magnetotails in our solar system A comparative approach to magnetotail phenomena, including reconnection, current sheet, rotation rate, Manufacturer: American Geophysical Union.

Online shopping for Books from a great selection of Electromagnetism, Dynamics, Mathematical Physics, Nuclear Physics, Mechanics, Solid-State Physics. A physics based model of the coupled magnetotail-ionosphere (Horton and Doxas, ) is used as an input–output filter, and its performance is compared to the Blanchard–McPherron database of isolated events.

Most model parameters can be calculated analytically for different substorm scenarios and closure schemes. Author: Vasyliūnas, Vytenis M.; Genre: Book Chapter; Published in Print: ; Title: Magnetotail: Unsolved Fundamental Problem of Magnetospheric Physics. The ISEE-1 and ISEE-2 observations of the lobe/mantle region and the plasma sheet boundary layer region at distances between 10 and 20 R E downstream during andhave been examined.

Cold, tailward flowing ionospheric 0 + streams observed during geomagnetically disturbed periods, have been statistically analysed.

At the crossing between the lobe/mantle region. The current sheet is a crucial region of the magnetotail, where a wide variety of energy conversion processes take place.

Large-amplitude vertical flapping oscillations of the current sheet are. Books Advanced Search New Releases Best Sellers & More Children's Books Textbooks Textbook Rentals Best Books of the Month of over 2, results for Books: Science & Math: Physics: Electromagnetism: Magnetism.

One substorm-associated magnetotail phenomenon is the formation of a large-scale plasmoid between the near-Earth and the distant X-lines and the subsequent injection tailward into the solar wind (e.g., Slavin et al.

). As for Mercury, large plasmoids are occasionally observed in the near magnetotail (Zhong et al. ).ISBN: OCLC Number: Description: x, pages: illustrations (chiefly color) ; 29 cm.

Contents: Preface / Andreas Keiling, Caitríona Jackman, and Peter Delamere --Section I: otail: Unsolved Fundamental Problem of Magnetospheric Physics / Vytenis M. Vasyliūnas --Section II: y's Magnetotail / T.

Sundberg and J.A. Slavin.The solar wind does not impact Earth directly but is deflected—like a stream diverted around a boulder—by our planet’s magnetic field, which forms a tear-drop-shaped cavity in the solar wind cavity—the magnetosphere—contains highly dilute plasmas whose behavior is controlled by Earth’s magnetic field and its interaction with the solar wind.