UpComing Seminars Recent Seminars | Dr Antonio Lei
On the Finiteness of Selmer groups Dr Byoung Du Kin
The congruences of congruent modular forms for non-ordinary primes
Dr Ernesto Nungesser
The future of some homogeneous spacetimes with an ensemble of free falling particles Professor Alan Coley
Persistence of black holes through
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Prof. Heiko Knospe
Nonstandard methods in p-adic analysis
Patrick Noble
A Bayesian Method for Forecasting Solar Cycles Using a Fokker-Planck Equation Woei Chet Lim
BKL singularity, spikes and inhomogeneous cosmology Emeritus Prof. R. Delbourgo
The big physics questions –
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Dr Daniel Delbourgo
How fast do solutions to polynomial equations grow?
Lyndon Embling (MSc student)
Axiomitisations of some Quasi-Ordered
Functions Semigroups using Determinative Pairs
Craig Armstrong (PhD student)
Modeling solar loop-top electron transport
using stochastic methods
Professor Geoffrey Grimmett - 2012 FORDER LECTURER
Conformality and universality in probability
Juri Toomre
Touching the inside of a convecting star and its magnetic dynamo Professor Florian Luca
Sierpinski and Riesel numbers and their friends
Dr Nick Cavenagh
A comparative study of defining sets in designs
Assoc. Prof. Steven Galbraith
Euclid's algorithm, continued fractions, factoring and the approximate GCD problem Dr Peter Kritzer
Uniformly Distributed Point Sets and Their Application to Quasi-Monte Carlo Algorithms
Dr Marcel Jackson
Constraint Satisfaction Problems and Universal Algebra
Dr Timothy Stokes
Comparison Semigroups and Function Algebra
Professor Ben Green
Arithmetic progressions of primes
Professor Ben Green
Linear equations in primes
Professor Roger Hosking
From Cold Regions to Modern Railtracks Dr Nicholas Cavenagh YouTube presentation Professor T.G. Forbes Predicting the Onset of Solar Eruptions Associate Professor Graeme Hocking
Coating deformations in the jet stripping process Andy Drizen
Finding Uniformly Distributed Steiner Triple Systems
Dr Nicholas Cavenagh
Cryptography, latin squares and cutting up triangles
Professor Stan Owocki
What Physics Sets the Upper Mass (Eddington) Limit of Stars? Professor Jongchul Chae Unsolved Problems in Solar Prominences
Dr Timothy Stokes Programs as Algebras Associate Professor Kevin Broughan
Three topics in number theory from 2008: the factorial function, flat primes and Lehmer's Euler phi function conjecture Associate Professor Graeme Hocking
A steady flow with unsteady forcing
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Comparison with CLUSTER data.
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Recent Seminars |
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University of Waikato 2004-04-23 G3.33 The Earth magnetosphere is a complex and highly dynamic system. Thanks to the CLUSTER mission launched in 2000, a 3D-picture of this magnetized environment is now available. Particularly, low frequency fluctuations are observed in some key-regions of the magnetosphere known as current sheets (magnetopause, magnetotail...). Such oscillations are also measured in the solar atmosphere where current sheets may form. In order to identify the nature of these perturbations and to explicit their role in the more global dynamics of the system, it is necessary to build a self-consistent model that studies theoretically the response of a current sheet to various excitations.
In this talk, I present an analysis of the propagation of compressive MHD perturbations in the Earth magnetotail (described as being an Harris-type sheet). I solve explicitly the linear response of the plasmasheet to an initial perturbation (initial displacement or external driver) by using the Green formalism. Two kinds of eigenmodes are found: global discrete oscillations of the plasmasheet and continuous localized oscillations that may transfer energy to the plasma through the resonant absorption process.
The theoretical model is then compared to a particular CLUSTER event, when the tetrahedron crossed the plasmasheet. The analysis of the observed fluctuations is carried out with the aim of determining if they are MHD global eigenmodes. If most of the low frequency oscillations do not match the theoretical eigenmodes of the plasmasheet, some higher frequency oscillations linked to a substorm agree remarkably well with the linear response of the sheet to an initial vertical displacement. However, a last perturbation at 0.04Hz is not explained by the MHD model and may represent the first experimental evidence of a tearing mode. |
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