3 edition of Some contributions to knowledge of the magnetospheric plasma by ISEE investigators found in the catalog.
Some contributions to knowledge of the magnetospheric plasma by ISEE investigators
by National Aeronautics and Space Administration, Goddard Space Flight Center in Greenbelt, Md
Written in English
|Series||NASA technical memorandum -- 86124|
|Contributions||Goddard Space Flight Center|
|The Physical Object|
field to maintain pressure balance in the plasma; 2) the response of the magnetic field to currents in the plasma and 3) Europa’s plasma exosphere and atmosphere. Estimates of the plasma pressure contribution to the magnetic field measurements range from ~20 nT in the magnetospheric lobes to over nT within the plas-ma sheet. Abstract The results of the Promiks-1 experiment to investigate the mass and energetic properties of the magnetospheric plasma are reviewed. The experiment was carried out on board the Prognoz-7 spacecraft in the vicinity of the ring current and the high-latitude magnetospheric boundary. A few examples of prolonged (up to 10 h in duration) steady magnetospheric convection (SMC) are studied here. The plasma and magnetic field measurements on board the ISEE-1 spacecraft (at X ≈ −20 R E near its apogee) displayed the stable plasma sheet (PS) configuration and steady earthward plasma convection that are essential elements of SMC by: Unfortunately, this book can't be printed from the OpenBook. If you need to print pages from this book, we recommend downloading it as a PDF. Visit to get more information about this book, to buy it in print, or to download it as a free PDF.
3 Magnetospheric simulation and prediction of the plasma environment Real-time magnetospheric simulation NICT is conducting magnetospheric simu-lation in real time by using the calculative approach of three-dimensional magneto-hydrodynamics (MHD). Figure 1 . The plasma magnet consists of a pair of polyphase coils that produce a rotating magnetic field (RMF) that drives the necessary currents in the plasma to inflate and maintain the large-scale magnetic structure. The plasma magnet is deployed by the Lorentz self-force on the plasma currents, expanding outward in a disk-like shape until theFile Size: 2MB. Plasma pressure data from the ISEE 2 fast plasma experiment (FPE) were statistically analyzed to determine the plasma sheet pressure versus distance in the midnight local time sector of the near-earth (12–35 RE) magnetotail plasma sheet. The observed plasma pressure, assumed isotropic, was mapped along model magnetic field flux tubes (obtained from the Tsyganenko and Usmanov  model) to Cited by: Abstract.- 1 Introduction.- 2 Outline.- 3 Two Problems of Coupled Spatial Transport and Pitch Angle Diffusion.- Radiation Belt Diffusion and Loss.- The Diffuse Aurora.- 4 General Properties of Electrostatic Waves in a Magnetized Plasma.- Linear Dispersion Relation.- Separable Distribution Functions.- Electrostatic Waves in a Zero Temperature Plasma.- Bernstein .
Plasma populations throughout the universe interact with solid bodies, gases, magnetic fields, electromagnetic radiation, magnetohydrodynamic waves, shock waves, and other plasma populations. These interactions can occur locally as well as on very large . ADS Classic is now deprecated. It will be completely retired in October Please redirect your searches to the new ADS modern form or the classic info can be found on our blog. Mini-Magnetospheric Plasma Propulsion (M2P2) is an advanced plasma propulsion system that will enable spacecraft to attain unprecedented speeds, with minimal energy and mass requirements. The high efficiency and specific impulse attained by the system is due to its utilization of ambient energy, in this case the energy from the solar wind, to. Understanding of the plasma depletion process in the dayside magnetosheath, the nature of magnetotail boundary motion, and the geometry of the magnetospheric.
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Get this from a library. Some contributions to knowledge of the magnetospheric plasma by ISEE investigators. [K W Ogilvie; Goddard Space Flight Center.]. The ISEE project has made substantial contributions to the knowledge of the magnetosphere during the period of the IMS, especially in the discipline of Space Plasma Physics.
Results obtained during approximately the first two years of the operation of ISEE-1 and -2, and touches on relevant results of ISEE-3 are : K.
Ogilvie. Precursors to interplanetary shocks are also observed. Inside the magnetosphere, ISEE contributed to knowledge of plasma waves, and, augmenting work with GEOS, to studies of plasma composition. In the near tail, the boundary layer of the plasma sheet disclosed interesting phenomena.
Precursors to interplanetary shocks are also observed. Inside the magnetosphere, ISEE contributed to knowledge of plasma waves, and, augmenting work with GEOS, to studies of plasma composition. In the near tail, the boundary layer of the plasma sheet disclosed interesting phenomenaAuthor: K.
Ogilive. The ISEE project has made Some contributions to knowledge of the magnetospheric plasma by ISEE investigators book contributions to the knowledge of the magnetosphere during the period of the IMS, especially in the discipline of Space Plasma Physics.
Results obtained during approximately the first two years of the operation of ISEE-1 and -2, and touches on relevant results of ISEE-3 are reviewed. the major contributions by isee-1 and -2 to the knowledge of magnetospheric plasmas include: • mapping the structure of the earth's foreshock, and bringing the study of the phenomena there to the level of fundamental physical processes.
• demonstrating reconnection, steady state at the magnetopause and transient at flux. ResultsfromtheGeos-1andGeos-2spacecraftandtheir contributionstotheIMS 9 Some contributions to knowledge ofthe magnetospheric plasmaby ISEE-1 investigators.
Some contributions to knowledge of the magnetospheric plasma by ISEE investigators book Contributions to the Terrestrial Magnetic Field W. Baumjohann and R. Nakamura, Space Research Institute, Austrian Academy of Sciences, Graz, mal energies above some K. Thus, a typical plasma is a hot and highly ionized gas.
While only a 78 Magnetospheric Contributions to the Terrestrial Magnetic Size: KB. Some are directed more toward the interests of laboratory plasma physics, like Chen’s book, others are highly mathematical, such that it would have required an additional course in applied.
A series of recent measurements of the outflow of ionization from the ionosphere have further heightened our awareness of the strength of the ionospheric source of magnetospheric plasmas.
In this paper the ionospheric contribution of the polar wind and cleft ion fountain at energies less than 10 eV has been added to the previously measured Cited by: Magnetospheric Plasma Physics.
Editors: Nishida, A. (Ed.) Earthquake prediction that was the business of astrologers and fortune-tellers some twenty years ago, has now grown up to be an important science.
*immediately available upon purchase as print book shipments may be delayed due to the COVID crisis. ebook access is temporary and. The book is the outcome of a three year long process. In December the study project on 'Source and Loss Processes of Magnetospheric Plasma' was se lected by ISSI after consultations with several groups of senior representatives of the space physics community.
This book provides a broad introduction to the kinetic theory of space plasma physics with the major focus on the inner magnetospheric plasma. It is designed to provide a comprehensive description of the different kinds of transport equations for both plasma particles and waves with an emphasis on the applicability and limitations of each set.
Margaret Galland Kivelson, Fran Bagenal, in Encyclopedia of the Solar System (Second Edition), Sources of Magnetospheric Plasmas. Magnetospheres contain considerable amounts of plasma, electrically charged particles in equal proportions of positive charge on ions and negative charge on electrons, from various sources.
The main source of plasma in the solar system is the Sun. This book addresses the electrical coupling between the hot, but dilute, magnetospheric plasma and the cold, but dense, plasma in the ionosphere.
In five major chapters, this book presents: basic properties of magnetosphere-ionosphere coupling; - morphology of electric fields and currents at high latitudes; - global modeling of magnetosphere. of magnetospheric structure, and is de-signed to make a large contribution to the International Magnetospheric Study (5).
The major parameters of the three spacecraft are set out in Table 1. Two of the spacecraft, ISEE-A and ISEE-B (known as the mother and daughter spacecraft, respectively), will be separated by a relatively small, con Cited by: mass, energy and momentum to the magnetospheric plasma population. Like-wise, magnetospheric particles can escape along ﬁeld lines.
This two-way transfer across the magnetopause continues while the ﬂux tube convects tailward with the external plasma ﬂow.
Figure schematically illustrates the geometry in the vicinity of the X-line. Knowledge of the ion composition in the near-Earth's magnetosphere and plasma sheet is essential for the understanding of magnetospheric processes and instabilities.
2 Microinstabilities of the Quiet Magnetospheric Tail The Lower-Hybrid-Drift Instability of the Plasma Sheet and the Anomalous Resistivity Pitch Angle Scattering Modulation by Plasma Convection. 3 Tearing Instability of the Magnetospheric Tail as the Mechanism for Substorms Energetics of Substorms Abstract.
The purpose of this chapter is to review briefly present knowledge on the distribution of plasmas in the magnetosphere and to attempt to find the link between magnetospheric Cited by: 2.
Magnetospheric plasma physics. A. Nishida (Editor).Developments in Earth and Planetary SciencesCited by: The ISEE-1 and ISEE-3 spacecraft were the principal contributions of NASA, while ISEE-2 was built and managed by ESA.
More than investigators, representing most of the magnetospheric community, from 33 institutes were involved in the ISEE mission and its 32 instruments.magnetospheric and near-Earth solar ebook plasma is the cause of many phenomena in the magnetosphere and the ebook, and a ects the way in which we observe many other features.
For many years, scientists have tried to understand the physical phenomena in-volved in the transfer of plasma from the solar wind into the magnetosphere andFile Size: 3MB.