Physics of Solar Planetary Environments: Vols. I & II PDF Download

Author:
Publisher: American Geophysical Union
ISBN:
Category :
Languages : en
Pages : 523

View

Book Description

Author: Tadanori Ondoh
Publisher: IOS Press
ISBN: 9784274903847
Category : Atmosphere, Upper
Languages : en
Pages : 322

View

Book Description

Author: Tamas I. Gombosi
Publisher: Cambridge University Press
ISBN: 052159264X
Category : Science
Languages : en
Pages : 361

View

Book Description
This book provides a comprehensive introduction to the physical phenomena that result from the interaction of the sun and the planets - often termed space weather. Physics of the Space Environment explores the basic processes in the Sun, in the interplanetary medium, in the near-Earth space, and down into the atmosphere. The first part of the book summarizes fundamental elements of transport theory relevant for the atmosphere, ionosphere and the magnetosphere. This theory is then applied to physical phenomena in the space environment. The fundamental physical processes are emphasized throughout, and basic concepts and methods are derived from first principles. This book is unique in its balanced treatment of space plasma and aeronomical phenomena. Students and researchers with a basic mathematics and physics background will find this book invaluable in the study of phenomena in the space environment.

Author: Rainer Schwenn
Publisher: Springer Science & Business Media
ISBN: 3642753647
Category : Science
Languages : en
Pages : 360

View

Book Description
Physics of the Inner Heliosphere gives for the first time a comprehensive and complete summary of our knowledge of the inner solar system. Using data collected over more than 11 years by the HELIOS twin solar probes, one of the most successful ventures in unmanned space exploration, the authors have compiled six extensive reviews of the physical processes of the inner heliosphere and their relation to the solar atmosphere. Researchers and advanced students in space and plasma physics, astronomy, and solar physics will be surprised to see just how closely the heliosphere is tied to, and how sensitively it depends on, the sun. Volume 2 deals with particles, waves, and turbulence, with chapters on: - magnetic clouds - interplanetary clouds - the solar wind plasma and MHD turbulence - waves and instabilities - energetic particles in the inner solar system

Author: J.G. Roederer
Publisher: Springer Science & Business Media
ISBN: 940097096X
Category : Science
Languages : en
Pages : 415

View

Book Description
Solar-Terrestrial Physics: The Study of Mankind's Newest Frontier Solar-Terrestrial Physics (STP) has been around for 100 years. However, it only became known as a scientific discipline under that name when the physical domain studied by STP became accessible to in situ observation and measurement by man or man-made instruments. Indeed, it was STP that provided the initial scientific driving force for the launching of man-made devices into extra-terrestrial space during the International Geophysical Year - aided of course by the genetically engrained drive of humans to expand their frontiers of knowledge, influence and dominance. We may define STP as the discipline dealing with the variable components of solar corpuscular and electromagnetic emissions, the physical processes governing their sources and their propagation through interplanetary space, and the physical-chemical processes related to their interaction with the Earth and other bodies in interplanetary space. Much of STP deals with fully-or partially-ionized gas flows and related energy, momentum and mass transfer in what now appears as one single system made up of distinct but strongly interacting parts, reaching from the photosphere out to the confines of the heliopause, engulfing planets and other solar system bodies, and dipping deep into 6 the Earth's atmosphere.

Author: Andreas Keiling
Publisher: John Wiley & Sons
ISBN: 1118842340
Category : Science
Languages : en
Pages : 417

View

Book Description
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.

Author: Eugene F. Milone
Publisher: Springer Science & Business Media
ISBN: 0387731555
Category : Science
Languages : en
Pages : 266

View

Book Description
It presents equations and derivations starting from a level that permits one to see the underlying physical ideas. There is no other book that does this on the market. The book presents an up-to-date overview on all essential topics but is concise where possible to keep it a practical resource for courses. The book is based on extensive experience in the class room. Its contents have been field-tested for years by students.

Author: J. Lemaire
Publisher: Pergamon
ISBN:
Category : Science
Languages : en
Pages : 100

View

Book Description

Author:
Publisher:
ISBN:
Category : Laboratories
Languages : en
Pages : 954

View

Book Description

Author: André Balogh
Publisher: Springer Science & Business Media
ISBN: 148997413X
Category : Science
Languages : en
Pages : 631

View

Book Description
Presents a comprehensive review of physical processes in astrophysical plasmas. This title presents a review of the detailed aspects of the physical processes that underlie the observed properties, structures and dynamics of cosmic plasmas. An assessment of the status of understanding of microscale processes in all astrophysical collisionless plasmas is provided. The topics discussed include turbulence in astrophysical and solar system plasmas as a phenomenological description of their dynamic properties on all scales; observational, theoretical and modelling aspects of collisionless magnetic reconnection; the formation and dynamics of shock waves; and a review and assessment of microprocesses, such as the hierarchy of plasma instabilities, non-local and non-diffusive transport processes and ionisation and radiation processes. In addition, some of the lessons that have been learned from the extensive existing knowledge of laboratory plasmas as applied to astrophysical problems are also covered. This volume is aimed at graduate students and researchers active in the areas of cosmic plasmas and space science. Originally published in Space Science Reviews journal, Vol. 278/2-4, 2013.