Award Abstract # 1104364
Spatiotemporal Development and Forecasting of Space Storms

NSF Org: AGS
Division of Atmospheric and Geospace Sciences
Recipient: PRESBYTERIAN COLLEGE
Initial Amendment Date: March 6, 2012
Latest Amendment Date: August 27, 2013
Award Number: 1104364
Award Instrument: Continuing Grant
Program Manager: Michael Wiltberger
AGS
 Division of Atmospheric and Geospace Sciences
GEO
 Directorate for Geosciences
Start Date: March 15, 2012
End Date: February 28, 2017 (Estimated)
Total Intended Award Amount: $217,194.00
Total Awarded Amount to Date: $217,194.00
Funds Obligated to Date: FY 2012 = $71,433.00
FY 2013 = $145,761.00
History of Investigator:
  • James Wanliss (Principal Investigator)
Recipient Sponsored Research Office: Presbyterian College
503 S BROAD ST
CLINTON
SC  US  29325-2998
(864)833-8489
Sponsor Congressional District: 03
Primary Place of Performance: Presbyterian College
503 S BROAD ST
CLINTON
SC  US  29325-2998
Primary Place of Performance
Congressional District:
03
Unique Entity Identifier (UEI): ZA5MNASDKUN3
Parent UEI: ZA5MNASDKUN3
NSF Program(s): MAGNETOSPHERIC PHYSICS
Primary Program Source: 01001314DB NSF RESEARCH & RELATED ACTIVIT
01001213DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 9196, 9150, OTHR
Program Element Code(s): 575000
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.050

ABSTRACT

This project will apply and extend two new approaches to the problem of recasting magnetic storms. In particular it will develop tools for forecasting of extreme events in ground-based magnetic indices. It will also develop tools for accurately predicting local magnetic fluctuations on the ground that are generated by magnetic storms. Local forecasts during and prior to storms are particularly important since coupling of the magnetosphere-ionosphere system produces geospace and ground magnetic variations whose statistical properties vary with both local time and latitude. The project will develop risk estimation methods based on (1) the statistics of the waiting times between storms above (below) a certain threshold, and (2) a symbolic dynamics method which quantifies temporal variations in the magnetic fluctuations and incorporates the solar wind driving fluctuations. Recent years have witnessed the development of tools that allow for the analysis of data that feature sudden transitions and extreme events, like space storms. These advances have been made possible by a combination of approaches based on dynamical systems theory and statistical physics. A growing catalogue of research provides evidence that the magnetosphere behaves like a complex system with sudden transitions and extreme events that have a distinct statistical structure, including heavy-tailed Levy-type behavior. Because of this complex nature it is possible to leverage the data statistics to make probabilistic hazard assessments for storm risk. These are primarily based on the association of small disturbances with future large storms. The project will examine the way in which the nonlinear behavior in the driver and the magnetosphere interact to produce space storms, especially those for which there is no obvious gross trigger.

American society relies upon technologies such as power distribution systems and constellations of communications satellites for its daily functioning. These technologies are all susceptible to the effects of magnetic storms (also called space storms). Increased societal dependence on these technologies implies the need to understand and predict spatiotemporal fluctuations in the magnetosphere. In addition to the improved ability to predict important space weather phenomena the project will include meaningful research performed by undergraduate students.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

Note:  When clicking on a Digital Object Identifier (DOI) number, you will be taken to an external site maintained by the publisher. Some full text articles may not yet be available without a charge during the embargo (administrative interval).

Some links on this page may take you to non-federal websites. Their policies may differ from this site.

Wanliss, J.A., K. Shiokawa, and K. Yumoto "Latitudinal variation of stochastic properties of the geomagnetic field" JournalNonlin. Processes Geophys. , v.21 , 2014 , p.347 Nonlin. Processes Geophys.,
Wanliss, J.A., K. Shiokawa, and K. Yumoto "Stochastic properties of the geomagnetic field across the 210 mm chain" Nonlinear Processes in Geophysics , v.21 , 2014 , p.1 10.5194/npg-21-1-2014
Dobias, P. and J.A. Wanliss "Interdisciplinary Applications of Statistical Physics to Modeling Decisions in Combat Situations" Intl. J. Arts and Sci.Intl. J. Arts and Sci , v.7 , 2014 , p.271
Wanliss, J. A., and P. Dobias "Empirical Mode Decomposition Applied to Afghanistan Violence Data: Comparison with Multiplicative Seasonal Decomposition" J. Battlefield Tech. , v.17 , 2014 , p.17 1440-5113
Wanliss, J. A., and P. Dobias. "Dealing with Non-Stationarities in Violence data using Empirical Mode Decomposition" J. Battlefield Tech. , v.16 , 2013 , p.9 1440-5113
Dobias, P. and J.A. Wanliss "Interdisciplinary Applications of Statistical Physics to Modeling Decisions in Combat Situations" Intl. J. Arts and Sci. , v.7 , 2014 , p.271 1943-6114

Please report errors in award information by writing to: awardsearch@nsf.gov.

Print this page

Back to Top of page