Magnetism Planetary Rotation And Convection In The Solar System

Magnetism Planetary Rotation And Convection In The Solar System Book in PDF, ePub and Kindle version is available to download in english. Read online anytime anywhere directly from your device. Click on the download button below to get a free pdf file of Magnetism Planetary Rotation And Convection In The Solar System book. This book definitely worth reading, it is an incredibly well-written.

Magnetism, Planetary Rotation, and Convection in the Solar System: Retrospect and Prospect

Author : W. O'Reilly
Publisher : Springer Science & Business Media
Page : 409 pages
File Size : 42,7 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400954045

Get Book

Magnetism, Planetary Rotation, and Convection in the Solar System: Retrospect and Prospect by W. O'Reilly Pdf

On the 6th, 7th' and 8th April 1983, a conference entitled "Magnetism, planetary rotation and convection in the Solar System" was held in the School of Physics at the University of Newcastle upon Tyne. The purpose of the meeting was to celebrate the 60th birthday of Prof. Stanley Keith Runcorn and his, and his students' and associates', several decades of scientific achievement. The social programme, which consisted of excursions in Northumberland and Durham with visits to ancient castles and churches, to Hexham Abbey and Durham Cathedral, and dinners in Newcastle and Durham, was greatly enjoyed by those attending the meeting and by their guests. The success ofthe scientific programme can be judged by this special edition of Geophysical Surveys which is derived mainly from the papers given at the meeting. The story starts in the late 1940s when the question of the origin of the magnetic field of the Earth and such other heavenly bodies as had at that time been discovered as having a magnetic field, was exercising the minds of several scientists; notably P. M. S. Blackett at Manchester, W. M. Elsasser at the University of Pennsylvania and E. C. Bullard at Cambridge. Two alternative mechanisms were proposed. In one the magnetic field was in some way connected with the distributed angular momentum of a rotating body; in the other, electric currents in conducting parts within the body were proposed as the source of magnetic field.

Magnetic Fields in the Solar System

Author : Hermann Lühr,Johannes Wicht,Stuart A. Gilder,Matthias Holschneider
Publisher : Springer
Page : 413 pages
File Size : 47,7 Mb
Release : 2018-01-10
Category : Science
ISBN : 9783319642925

Get Book

Magnetic Fields in the Solar System by Hermann Lühr,Johannes Wicht,Stuart A. Gilder,Matthias Holschneider Pdf

This book addresses and reviews many of the still little understood questions related to the processes underlying planetary magnetic fields and their interaction with the solar wind. With focus on research carried out within the German Priority Program ”PlanetMag”, it also provides an overview of the most recent research in the field. Magnetic fields play an important role in making a planet habitable by protecting the environment from the solar wind. Without the geomagnetic field, for example, life on Earth as we know it would not be possible. And results from recent space missions to Mars and Venus strongly indicate that planetary magnetic fields play a vital role in preventing atmospheric erosion by the solar wind. However, very little is known about the underlying interaction between the solar wind and a planet’s magnetic field. The book takes a synergistic interdisciplinary approach that combines newly developed tools for data acquisition and analysis, computer simulations of planetary interiors and dynamos, models of solar wind interaction, measurement of ancient terrestrial rocks and meteorites, and laboratory investigations.

Solar System Magnetic Fields

Author : E.R. Priest
Publisher : Springer Science & Business Media
Page : 302 pages
File Size : 49,9 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400954823

Get Book

Solar System Magnetic Fields by E.R. Priest Pdf

In September 1984 a Summer School on Solar System Plasmas was held at Imperial College with the support of the Science and Engineering Research Council. An excellent group of lecturers was assembled to give a series of basic talks on the various aspects of the subject, aimed at Ph. D. students or researchers from related areas wanting to learn about the plasma physics of the solar system. The students were so appreciative of the lectures that it was decided to write them up as the present book. Traditionally, different areas of solar system science, such as solar and magnetospheric physics, have been studied by separate communities with little contact. However, it has become clear that many common themes cut right across these distinct topics, such as magnetohydrodynamic instabilities and waves, magnetic reconnect ion , convection, dynamo activity and particle acceleration. The plasma parameters may well be quite different in the Sun's atmosphere, a cometary tailor Jupiter's magnetosphere, but many of the basic processes are similar and it is by studying them in different environments that we come to understand them more deeply. Furthermore, direct in situ measurements of plasma properties at one point in the solar wind or the magnetosphere complement the more global view by remote sensing of a similar phenomenon at the Sun.

Planetary Magnetism

Author : U.R. Christensen,Andre Balogh,Doris Breuer,Karl-Heinz Glaßmeier
Publisher : Springer
Page : 668 pages
File Size : 50,7 Mb
Release : 2012-10-13
Category : Science
ISBN : 1461426332

Get Book

Planetary Magnetism by U.R. Christensen,Andre Balogh,Doris Breuer,Karl-Heinz Glaßmeier Pdf

The articles in this volume cover, for the first time, all aspects of planetary magnetism, from the observations made by space missions to their interpretation in terms of the properties of all the planets in the solar system. Studies of dynamo-generated magnetic fields in Mercury, the Earth, the giant planets, as well as in Ganymede, one of Jupiter’s moons, are presented. Crustal magnetic field in Mars, the Mon and the Earth are described as well as magnetic fields induced in the solar system bodies. There are several articles dealing with dynamo theory and modelling and applications to the different planets.

Space Physics and Aeronomy, Magnetospheres in the Solar System

Author : Romain Maggiolo,Nicolas André,Hiroshi Hasegawa,Daniel T. Welling
Publisher : John Wiley & Sons
Page : 61 pages
File Size : 49,6 Mb
Release : 2021-05-04
Category : Science
ISBN : 9781119507529

Get Book

Space Physics and Aeronomy, Magnetospheres in the Solar System by Romain Maggiolo,Nicolas André,Hiroshi Hasegawa,Daniel T. Welling Pdf

An overview of current knowledge and future research directions in magnetospheric physics In the six decades since the term 'magnetosphere' was first introduced, much has been theorized and discovered about the magnetized space surrounding each of the bodies in our solar system. Each magnetosphere is unique yet behaves according to universal physical processes. Magnetospheres in the Solar System brings together contributions from experimentalists, theoreticians, and numerical modelers to present an overview of diverse magnetospheres, from the mini-magnetospheres of Mercury to the giant planetary magnetospheres of Jupiter and Saturn. Volume highlights include: Concise history of magnetospheres, basic principles, and equations Overview of the fundamental processes that govern magnetospheric physics Tools and techniques used to investigate magnetospheric processes Special focus on Earth’s magnetosphere and its dynamics Coverage of planetary magnetic fields and magnetospheres throughout the solar system Identification of future research directions in magnetospheric physics The American Geophysical Union promotes discovery in Earth and space science for the benefit of humanity. Its publications disseminate scientific knowledge and provide resources for researchers, students, and professionals. Find out more about the Space Physics and Aeronomy collection in this Q&A with the Editors in Chief

Magnetotails in the Solar System

Author : Andreas Keiling,Caitríona Jackman,Peter Delamere
Publisher : John Wiley & Sons
Page : 417 pages
File Size : 43,9 Mb
Release : 2015-02-02
Category : Science
ISBN : 9781118842348

Get Book

Magnetotails in the Solar System by Andreas Keiling,Caitríona Jackman,Peter Delamere Pdf

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. Mars and Venus have no global intrinsic magnetic field, yet they possess induced magnetotails. Comets have magnetotails that are formed by the draping of the interplanetary magnetic field. In the case of planetary satellites (moons), the magnetotail refers to the wake region behind the satellite in the flow of either the solar wind or the magnetosphere of its parent planet. The largest magnetotail of all in our solar system is the heliotail, the “magnetotail” of the heliosphere. The variety of solar wind conditions, planetary rotation rates, ionospheric conductivity, and physical dimensions provide an outstanding opportunity to extend our understanding of the influence of these factors on magnetotail processes and structures. Volume highlights include: Discussion on why a magnetotail is a fundamental problem of magnetospheric physics Unique collection of tutorials on a large range of magnetotails in our solar system In-depth reviews comparing magnetotail processes at Earth with other magnetotail structures found throughout the heliosphere Collectively, Magnetotails in the Solar System brings together for the first time in one book a collection of tutorials and current developments addressing different types of magnetotails. As a result, this book should appeal to a broad community of space scientists, and it should also be of interest to astronomers who are looking at tail-like structures beyond our solar system.

The Origin and Dynamics of Solar Magnetism

Author : M.J. Thompson,A. Balogh,J.L. Culhane,Å. Nordlund,S.K. Solanki,J.-P. Zahn
Publisher : Springer Science & Business Media
Page : 424 pages
File Size : 47,5 Mb
Release : 2009-05-01
Category : Science
ISBN : 9781441902399

Get Book

The Origin and Dynamics of Solar Magnetism by M.J. Thompson,A. Balogh,J.L. Culhane,Å. Nordlund,S.K. Solanki,J.-P. Zahn Pdf

Starting in 1995 numerical modeling of the Earth’s dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of approximately the right strength, they show spatial power spectra similar to that of Earth, and the magnetic eld morphology and the temporal var- tion of the eld resembles that of the geomagnetic eld (Christensen and Wicht 2007). Some models show stochastic dipole reversals whose details agree with what has been inferred from paleomagnetic data (Glatzmaier and Roberts 1995; Kutzner and Christensen 2002; Wicht 2005). While these models represent direct numerical simulations of the fundamental MHD equations without parameterized induction effects, they do not match actual pla- tary conditions in a number of respects. Speci cally, they rotate too slowly, are much less turbulent, and use a viscosity and thermal diffusivity that is far too large in comparison to magnetic diffusivity. Because of these discrepancies, the success of geodynamo models may seem surprising. In order to better understand the extent to which the models are applicable to planetary dynamos, scaling laws that relate basic properties of the dynamo to the fundamental control parameters play an important role. In recent years rst attempts have been made to derive such scaling laws from a set of numerical simulations that span the accessible parameter space (Christensen and Tilgner 2004; Christensen and Aubert 2006).

The New Solar System

Author : J. Kelly Beatty,Carolyn Collins Petersen,Andrew Chaikin
Publisher : Cambridge University Press
Page : 440 pages
File Size : 48,7 Mb
Release : 1999-01-28
Category : Science
ISBN : 0521645875

Get Book

The New Solar System by J. Kelly Beatty,Carolyn Collins Petersen,Andrew Chaikin Pdf

New edition of the leading planetary science textbook packed with the latest images, data, and results from recent planetary missions.

Mars’ Magnetism and Its Interaction with the Solar Wind

Author : Daniel Winterhalter,Mario Acuña,Alexander Zakharov
Publisher : Springer Science & Business Media
Page : 269 pages
File Size : 55,9 Mb
Release : 2013-06-05
Category : Science
ISBN : 9780306486043

Get Book

Mars’ Magnetism and Its Interaction with the Solar Wind by Daniel Winterhalter,Mario Acuña,Alexander Zakharov Pdf

Given that the question of an internal magnetic field is of fundamental importance to the understanding of Mars' formation and thermal evolution, and of the evolution of Mars' atmosphere, surprisingly few of the many spacecraft sent to Mars were equipped with instrumentation for such investigations. Of the 9 or so orbiters that have successfully archived Mars orbit, even if for a short period of time, only two have returned useful data about the magnetic field and about the plasma environment near Mars: The Phobos 2 spacecraft, and more recently, Mars Global Surveyor (MGS). With the discovery by MGS that Mars has large remnant magnetic field structures indicating an internal dynamo long extinct, the true nature of the past and present interaction between Mars and the solar wind comes, for the first time, into sharp focus. This work, detailing the integration and new interpretation of the MGS and Phobos results, is a primary reference for the researcher studying solar wind/planet interactions.

The Cambridge Guide to the Solar System

Author : Kenneth R. Lang
Publisher : Cambridge University Press
Page : 503 pages
File Size : 50,7 Mb
Release : 2011-03-03
Category : Science
ISBN : 9781139494175

Get Book

The Cambridge Guide to the Solar System by Kenneth R. Lang Pdf

Richly illustrated with full-color images, this book is a comprehensive, up-to-date description of the planets, their moons, and recent exoplanet discoveries. This second edition of a now classic reference is brought up to date with fascinating new discoveries from 12 recent Solar System missions. Examples include water on the Moon, volcanism on Mercury's previously unseen half, vast buried glaciers on Mars, geysers on Saturn's moon Enceladus, lakes of hydrocarbons on Titan, encounter with asteroid Itokawa, and sample return from comet Wild 2. The book is further enhanced by hundreds of striking new images of the planets and moons. Written at an introductory level appropriate for undergraduate and high-school students, it provides fresh insights that appeal to anyone with an interest in planetary science. A website hosted by the author contains all the images in the book with an overview of their importance. A link to this can be found at www.cambridge.org/solarsystem.

Advances in Solar System Magnetohydrodynamics

Author : Eric Ronald Priest,Alan W. Hood
Publisher : Cambridge University Press
Page : 460 pages
File Size : 41,8 Mb
Release : 1991-06-28
Category : Mathematics
ISBN : 0521403251

Get Book

Advances in Solar System Magnetohydrodynamics by Eric Ronald Priest,Alan W. Hood Pdf

Most of the solar system is in the plasma state and its subtle non-linear interaction with the magnetic field is described for many purposes by the equations of magnetohydrodynamics (MHD). Over the past few years this important and complex field has become one of the most actively pursued areas of research, with increasingly diverse applications in geophysics, space physics and astrophysics. This book examines the basic MHD topics, such as equilibria, waves, instabilities and reconnection and examines each in the context of different areas that utilize MHD. Many of the world's leading experts have contributed to this volume, which has been edited by two of the key enthusiasts. It is hoped that it can help the reader to appreciate and understand the common threads between the different branches of magnetohydrodynamics. This book will be a timely exposition of recent advances made in the field.