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Started:09/26/2007
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Report:11/12/2009
Report:10/27/2008
Latest Quad:12/22/2006
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2008 Workshop Presentation
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...[Abstract]
PI: Jay Johnson
Princeton U

Novel Higher-Order Statistical Method for Extracting Dependencies in Multivariate Geospace Data Sets
Understanding magnetospheric dynamics and the relationship between the solar wind driver and the magnetospheric response is of great practical interest because it could potentially help to avert catastrophic loss of power and communications. In order to build good predictive models it is necessary to understand the most critical nonlinear dependencies among observed plasma and electromagnetic field variables in the coupled solar wind/magnetosphere system. We propose to develop and apply a novel cumulant-based information-dynamical measure in conjunction with other nonlinear techniques to magnetospheric data to characterize: (1) the underlying dynamics, (2) the nonlinear behavior of the geospace systems, (3) the solar cycle dependence of these properties, and (4) the predictability of the systems. Because this nonparametric, statistical approach assumes no intrinsic underlying dynamics, it is possible to avoid some of the pitfalls involved in parametric modeling and/or physics based models. Moreover, the information gained from the cumulant-based information flow could be used to guide the development of predictive models. To illustrate the power of our method, we will examine the nonlinear cross dependencies in a large database of geospace variables. We will evaluate the underlying dynamics of the magnetosphere by examining the time evolution of geomagnetic indices, Kp, Dst, and AE, as well as more direct measures of the magnetospheric state, energetic electron flux, tail stretching, and energetic electron precipitation. From this data we will be able to estimate a predictability horizon which will indicate the maximum ``look ahead'' for which the space climate can be predicted. We will also use the information-dynamical measures to identify variables derived from solar wind data that maximize the information content about the magnetospheric response. This work should have a significant impact on space science, space/mathematical science education, and society at large. First, we have developed a new technique for analyzing nonlinear dependencies in large data set using cumulant-based significance measures. Because the methods and techniques do not presuppose an underlying dynamics, they are transportable across a wide range of complex nonlinear systems which can broadly impact fields ranging from geoscience to bioscience. Second, detection of the most important nonlinear interactions in the systems could be used to identify the most important physical processes that will aid development of physical models and predictive capabilities for understanding severe space weather. Third, we will submit an E/PO proposal where we will develop web-based outreach tools to teach high school students basic concepts in nonlinear dynamics with applications to space science. Finally, the results will be widely disseminated in mathematical and geospace journals and presented at meetings and workshops.

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