Plasma Depletions In The Jovian Magnetosphere
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Time-variable Phenomena in the Jovian System
Author | : M. J. S. Belton |
Publisher | : |
Total Pages | : 420 |
Release | : 1989 |
Genre | : Jupiter (Planet) |
ISBN | : |
Plasma Sources of Solar System Magnetospheres
Author | : Andrew F. Nagy |
Publisher | : Springer |
Total Pages | : 296 |
Release | : 2016-01-27 |
Genre | : Science |
ISBN | : 1493935445 |
This volume reviews what we know of the corresponding plasma source for each intrinsically magnetized planet. Plasma sources fall essentially in three categories: the solar wind, the ionosphere (both prevalent on Earth), and the satellite-related sources. Throughout the text, the case of each planet is described, including the characteristics, chemical composition and intensity of each source. The authors also describe how the plasma generated at the source regions is transported to populate the magnetosphere, and how it is later lost. To summarize, the dominant sources are found to be the solar wind and sputtered surface ions at Mercury, the solar wind and ionosphere at Earth (the relative importance of the two being discussed in a specific introductory chapter), Io at Jupiter and – a big surprise of the Cassini findings – Enceladus at Saturn. The situation for Uranus and Neptune, which were investigated by only one fly-by each, is still open and requires further studies and exploration. In the final chapter, the book offers a summary of the little we know of Uranus and Neptune, then summarizes in a comparative way what we know of plasma sources throughout the solar system, and proposes directions for future research.
Determination of Electron Density in the Jovian Magnetosphere from Galileo Plasma Wave Data
Author | : Benjamin H. Richards |
Publisher | : |
Total Pages | : 98 |
Release | : 2006 |
Genre | : Electron distribution |
ISBN | : |
The Juno Mission
Author | : Scott Bolton |
Publisher | : Springer |
Total Pages | : 644 |
Release | : 2018-09-14 |
Genre | : Science |
ISBN | : 9789402415599 |
The Juno mission to Jupiter is one of the most ambitious, daring and challenging solar system exploration missions ever conceived. Next to the Sun, Jupiter is the largest object in our solar system. As such, it is both a record and driver of the formation and evolution of the planets -- no other object in our solar system can tell us more about the origin of planetary systems. Understanding the details of giant planet formation, structure, composition and powerful magnetospheric environment required a new perspective close up and over the poles of Jupiter -- an orbit never before attempted. Juno was specifically designed for this challenge, entering into the harshest planetary environment known in the solar system. This volume describes the mission design, scientific strategies and instrument payload that enable Juno to peer deep into Jupiter’s atmosphere and reveal the fundamental process of the formation and early evolution of our solar system. In these papers, the Juno instrument teams describe their investigations, which include gravity radio science, microwave radiometers, magnetometers, an infrared imager auroral mapper, an ultraviolet imager and spectrograph, a visible light imager known as JunoCam, low and high energy particle detectors and plasma wave and radio electromagnetic sensors. The articles also describe a radiation monitoring experiment and the extensive laboratory measurements undertaken to assist with the analysis and interpretation of Juno’s pioneering investigation of Jupiter’s deep atmosphere. Originally published in Space Science Reviews, Volume 213, Issue 1-4, November 2017
Transport, Chaos And Plasma Physics 2
Author | : Benkadda Sadruddin |
Publisher | : World Scientific |
Total Pages | : 460 |
Release | : 1996-08-22 |
Genre | : |
ISBN | : 9814547743 |
Since the early developments of 'nonlinear science', plasma physics played a major role in its evolution: solitons, hamiltonian chaos, distinction between absolute and convective instabilities, and dynamics of coherent structures in turbulence. Understanding transport in plasmas is important for fusion devices but also for fundamental astrophysics, for fluid mechanics, for theoretical chemistry and engineering, and plasma processing in engineering.This second workshop gathered experts in plasma physics, nonlinear phenomena and mathematics. It aimed at enabling theoreticians, numericians and experimentalists in plasma turbulence to relate electromagnetic fluctuations, modes of self-organisation and transport processes. It may lead to developing new diagnostics and new methods for signal processing.
Physics of the Jovian Magnetosphere
Author | : A. J. Dessler |
Publisher | : Cambridge University Press |
Total Pages | : 572 |
Release | : 1983 |
Genre | : Science |
ISBN | : 9780521520065 |
A valuable reference work for those doing research in magnetospheric physics and related disciplines.
Plasma in the Jovian Magnetosphere
Author | : Christoph Goertz |
Publisher | : |
Total Pages | : 94 |
Release | : 1975 |
Genre | : Jupiter (Planet) |
ISBN | : |
Physics of Space: Growth Points and Problems
Author | : Nicole Meyer-Vernet |
Publisher | : Springer Science & Business Media |
Total Pages | : 378 |
Release | : 2011-06-28 |
Genre | : Science |
ISBN | : 940100904X |
Proceedings of the Second "Rencontres de l'observatoire", Observatoire de Paris, Meudon, France
Saturn in the 21st Century
Author | : Kevin H. Baines |
Publisher | : Cambridge University Press |
Total Pages | : 495 |
Release | : 2019 |
Genre | : Science |
ISBN | : 110710677X |
A detailed overview of Saturn's formation, evolution and structure written by eminent planetary scientists involved in the Cassini Orbiter mission.