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Author: Tamás I. Gombosi Publisher: Pergamon ISBN: Category : Science Languages : en Pages : 352
Book Description
Hardbound. The symposium consisted of 75 invited and contributed presentations about controversial and poorly understood phenomena related to the plasma environments of comets, weakly magnetized and non-magnetized solar system bodies with significant atmospheres. Understanding of the major physical and chemical processes controlling cometary plasma environments has greatly improved following the historic spacecraft encounters with comets Halley and Giacobini-Zinner. Pioneer Venus has provided detailed information about the plasma environment of Venus over a full solar cycle. The Phobos mission has also significantly enhanced our understanding of the Martian magnetosphere and its solar wind interaction. There is renewed interest in the solar wind interaction with our Moon and efforts are continuing toward further exploration of the plasma environments of Io, Titan and Triton. Although these bodies have vastly different plasma environments, there are severa
Author: Tamás I. Gombosi Publisher: Pergamon ISBN: Category : Science Languages : en Pages : 352
Book Description
Hardbound. The symposium consisted of 75 invited and contributed presentations about controversial and poorly understood phenomena related to the plasma environments of comets, weakly magnetized and non-magnetized solar system bodies with significant atmospheres. Understanding of the major physical and chemical processes controlling cometary plasma environments has greatly improved following the historic spacecraft encounters with comets Halley and Giacobini-Zinner. Pioneer Venus has provided detailed information about the plasma environment of Venus over a full solar cycle. The Phobos mission has also significantly enhanced our understanding of the Martian magnetosphere and its solar wind interaction. There is renewed interest in the solar wind interaction with our Moon and efforts are continuing toward further exploration of the plasma environments of Io, Titan and Triton. Although these bodies have vastly different plasma environments, there are severa
Author: National Research Council Publisher: National Academies Press ISBN: 9780309092159 Category : Science Languages : en Pages : 100
Book Description
Solar and space physics is the study of solar system phenomena that occur in the plasma state. Examples include sunspots, the solar wind, planetary magnetospheres, radiation belts, and the aurora. While each is a distinct phenomenon, there are commonalities among them. To help define and systematize these universal aspects of the field of space physics, the National Research Council was asked by NASA's Office of Space Science to provide a scientific assessment and strategy for the study of magnetized plasmas in the solar system. This report presents that assessment. It covers a number of important research goals for solar and space physics. The report is complementary to the NRC report, The Sun to the Earthâ€"and Beyond: A Decadal Research Strategy for Solar and Space Physics, which presents priorities and strategies for future program activities.
Author: C.T. Russell Publisher: Springer Science & Business Media ISBN: 0387709436 Category : Science Languages : en Pages : 503
Book Description
This book contains the latest results on the plasma environment of Mars and its interaction with the solar wind. These results include mapping of the plasma environment with the instruments on Mars Express and Mars Global Surveyor, the latest numerical simulations, and theoretical studies. This comprehensive examination of the Mars environment also sets the stage for the interpretation of the Venus Express measurements.
Author: U.R. Christensen Publisher: Springer ISBN: 9781461426332 Category : Science Languages : en Pages : 668
Book Description
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.
Author: Anil Bhardwaj Publisher: World Scientific ISBN: 9814475092 Category : Science Languages : en Pages : 234
Book Description
Advances in Geosciences is the result of a concerted effort in bringing the latest results and planning activities related to earth and space science in Asia and the international arena. The volume editors are all leading scientists in their research fields covering six sections: Hydrological Science (HS), Planetary Science (PS), Solar Terrestrial (ST), Solid Earth (SE), Ocean Science (OS) and Atmospheric Science (AS). The main purpose is to highlight the scientific issues essential to the study of earthquakes, tsunamis, atmospheric dust storms, climate change, drought, flood, typhoons, monsoons, space weather, and planetary exploration.
Author: National Research Council Publisher: National Academies Press ISBN: 0309313953 Category : Science Languages : en Pages : 37
Book Description
In 2010, NASA and the National Science Foundation asked the National Research Council to assemble a committee of experts to develop an integrated national strategy that would guide agency investments in solar and space physics for the years 2013-2022. That strategy, the result of nearly 2 years of effort by the survey committee, which worked with more than 100 scientists and engineers on eight supporting study panels, is presented in the 2013 publication, Solar and Space Physics: A Science for a Technological Society. This booklet, designed to be accessible to a broader audience of policymakers and the interested public, summarizes the content of that report.
Author: Stein Haaland Publisher: John Wiley & Sons ISBN: 111921632X Category : Science Languages : en Pages : 378
Book Description
DawnDusk Asymmetries in Planetary Plasma Environments Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other. For example, recent observations indicate that Earth's magnetopause is thicker at dawn than at dusk. Likewise, auroral breakups at Earth are more likely to occur in the pre-midnight than post-midnight sectors. Increasing availability of remotely sensed and in situ measurements of planetary ionospheres, magnetospheres and their interfaces to the solar wind have revealed significant and persistent dawn-dusk asymmetries. As yet there is no consensus regarding the source of many of these asymmetries, nor the physical mechanisms by which they are produced and maintained. Volume highlights include: A comprehensive and updated overview of current knowledge about dawn-dusk asymmetries in the plasma environments of planets in our solar system and the mechanisms behind them Valuable contributions from internationally recognized experts, covering both observations, simulations and theories discussing all important aspects of dawn-dusk asymmetries Space weather effects are caused by processes in space, mainly the magnetotail, and can be highly localized on ground. Knowing where the source, i.e., where dawn-dusk location is will allow for a better prediction of where the effects on ground will be most pronounced Covering both observational and theoretical aspects of dawn dusk asymmetries, Dawn-Dusk Asymmetries in Planetary Plasma Environments will be a valuable resource for academic researchers in space physics, planetary science, astrophysics, physics, geophysics and earth science.
Author: Steven W. Bougher Publisher: University of Arizona Press ISBN: 0816547904 Category : Science Languages : en Pages : 1377
Book Description
The final orbit of Venus by the Magellan spacecraft in October 1994 brought to a close an exciting period of Venus reconnaissance and exploration. The scientific studies resulting from data collected by the Magellan, Galileo, and Pioneer missions are unprecedented in their detail for any planet except Earth. Venus II re-evaluates initial assessments of Venus in light of these and other spacecraft missions and ground-based observations conducted over the past 30 years. More than a hundred contributors summarize our current knowledge of the planet, consider points of disagreement in interpretation, and identify priorities for future research. Topics addressed include geology, surface processes, volcanism, tectonism, impact cratering, geodynamics, upper and lower atmospheres, and solar wind environment. The diversity of the coverage reflects the interdisciplinary nature of Venus science and the breadth of knowledge that has contributed to it. A CD-ROM developed by the Jet Propulsion Laboratory accompanies the book and incorporates text, graphics, video, software, and various digital products from selected contributors to the text. A multimedia interface allows users to navigate the text and the extensive databases included on the disk. Venus II is the most authoritative single volume available on the second planet. Its contents will not only help shape the goals of future Venus missions but will also enhance our understanding of current Mars explorations.
Author: Tamás I. Gombosi
Author: Tamás I. Gombosi
Author: National Research Council
Author: C.T. Russell
Author: U.R. Christensen
Author: Anil Bhardwaj
Author: Robert M. Haberle
Author: National Research Council
Author: Stein Haaland
Author: Thomas E. Cravens
Author: Steven W. Bougher