Fast/Polar Conjunction Study of Field-Aligned Auroral Acceleration and Corresponding Magnetotail Drivers


Book Description

The discrete aurora results when energized electrons bombard the Earth's atmosphere at high latitudes. This paper examines the physical processes that can cause field-aligned acceleration of plasma particles in the auroral region. A data and theoretical study has been carried out to examine the acceleration mechanisms that operate in the auroral zone and to identity the magnetospheric drivers of these acceleration mechanisms. The observations used in the study were collected by the Fast Auroral SnapshoT (FAST) and Polar satellites when the two satellites were in approximate magnetic conjunction in the auroral region. During these events FAST was in the middle of the auroral zone and Polar was above the auroral zone in the near-Earth plasma sheet. Polar data was used to determine the conditions in the magnetotail at the time field-aligned acceleration was measured by FAST in the auroral zone. For each of the magnetotail drivers identified in the data study, the physics of field-aligned acceleration in the auroral region was examined using existing theoretical efforts and a long-system particle-in-cell simulation to model the magnetically connected region between the two satellites.Schriver, D. and Ashour-Abdalla, M. and Strangeway, R. J. and Richard, R. L. and Klezting, C. and Dotan, Y. and Wygant, J.Goddard Space Flight CenterAURORAL ZONES; POLAR REGIONS; ELECTRON ACCELERATION; PLASMA ACCELERATORS; ELECTRIC FIELDS; SATELLITE OBSERVATION; COMPUTERIZED SIMULATION; MAGNETOHYDRODYNAMIC WAVES




Auroral Phenomenology and Magnetospheric Processes


Book Description

Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 197. Many of the most basic aspects of the aurora remain unexplained. While in the past terrestrial and planetary auroras have been largely treated in separate books, Auroral Phenomenology and Magnetospheric Processes: Earth and Other Planets takes a holistic approach, treating the aurora as a fundamental process and discussing the phenomenology, physics, and relationship with the respective planetary magnetospheres in one volume. While there are some behaviors common in auroras of the different planets, there are also striking differences that test our basic understanding of auroral processes. The objective, upon which this monograph is focused, is to connect our knowledge of auroral morphology to the physical processes in the magnetosphere that power and structure discrete and diffuse auroras. Understanding this connection will result in a more complete explanation of the aurora and also further the goal of being able to interpret the global auroral distributions as a dynamic map of the magnetosphere. The volume synthesizes five major areas: auroral phenomenology, aurora and ionospheric electrodynamics, discrete auroral acceleration, aurora and magnetospheric dynamics, and comparative planetary aurora. Covering the recent advances in observations, simulation, and theory, this book will serve a broad community of scientists, including graduate students, studying auroras at Mars, Earth, Saturn, and Jupiter. Projected beyond our solar system, it may also be of interest for astronomers who are looking for aurora-active exoplanets.




Magnetospheric Plasma Physics: The Impact of Jim Dungey’s Research


Book Description

This book makes good background reading for much of modern magnetospheric physics. Its origin was a Festspiel for Professor Jim Dungey, former professor in the Physics Department at Imperial College on the occasion of his 90th birthday, 30 January 2013. Remarkably, although he retired 30 years ago, his pioneering and, often, maverick work in the 50’s through to the 70’s on solar terrestrial physics is probably more widely appreciated today than when he retired. Dungey was a theoretical plasma physicist. The book covers how his reconnection model of the magnetosphere evolved to become the standard model of solar-terrestrial coupling. Dungey’s open magnetosphere model now underpins a holistic picture explaining not only the magnetic and plasma structure of the magnetosphere, but also its dynamics which can be monitored in real time. The book also shows how modern day simulation of solar terrestrial coupling can reproduce the real time evolution of the solar terrestrial system in ways undreamt of in 1961 when Dungey’s epoch-making paper was published. Further contributions on current Earth magnetosphere research and space plasma physics included in this book show how Dungey’s basic ideas have remained explanative 50 years on. But the Festspiel also introduced some advances that possibly Dungey had not foreseen. One of the contributions presented in this book is on the variety of magnetospheres of the solar system which have been seen directly during the space age, discussing the variations in spatial scale and reconnection time scale and comparing them in respect of Earth, Mercury, the giant planets as well as Ganymede.




Annales Geophysicae


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Magnetospheric ULF Waves


Book Description

Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 169. Ultra-Low-Frequency (ULF) waves pervade the magnetosphere, a region shaped by the Earth's magnetic fieid and filled with an ionized gas known as plasma. As a mechanism for interaction of particles with fields and as a diagnostic tool for probing the structure of the magnetosphere, ULF waves are a rich medium for research and discovery. With new spacecraft and computer simulations, and ground-based magnetometers and radar networks, we have recently expanded our capacity to analyze ULF waves on a global scale with unprecedented precision. Magnetospheric ULF Waves: Synthesis and New Directions presents state-of-the-art information on ULF waves, and their effect on space weather, from three vantage points: Excitation and propagation Interaction with plasma and energetic particles Magnetospheric diagnostics Scientists, researchers, and students working in space physics, magnetospheric physics, atmospheric physics, climatoiogy and aeronomy will find this book an important resource for current and near-future investigations of the Sun-Earth relationship.










Spring Meeting


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Geomagnetism, Aeronomy and Space Weather


Book Description

An interdisciplinary review of research in geomagnetism, aeronomy and space weather, written by eminent researchers from these fields.




Solar and Space Physics


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.