NSF Org:	AGS Division of Atmospheric and Geospace Sciences
Recipient:	THE JOHNS HOPKINS UNIVERSITY
Initial Amendment Date:	August 7, 2007
Latest Amendment Date:	September 19, 2012
Award Number:	0720114
Award Instrument:	Continuing Grant
Program Manager:	Therese Moretto Jorgensen AGS  Division of Atmospheric and Geospace Sciences GEO  Directorate for Geosciences
Start Date:	September 1, 2007
End Date:	October 31, 2012 (Estimated)
Total Intended Award Amount:	$0.00
Total Awarded Amount to Date:	$299,849.00
Funds Obligated to Date:	FY 2007 = $99,942.00 FY 2008 = $99,928.00 FY 2009 = $99,979.00
History of Investigator:	Brian Anderson (Principal Investigator) brian.anderson@jhuapl.edu Joseph Baker (Co-Principal Investigator) Haje Korth (Co-Principal Investigator) Yihua Zheng (Co-Principal Investigator)
Recipient Sponsored Research Office:	Johns Hopkins University 3400 N CHARLES ST BALTIMORE MD  US  21218-2608 (443)997-1898
Sponsor Congressional District:	07
Primary Place of Performance:	Johns Hopkins University Applied Physics Laboratory 11100 JOHNS HOPKINS RD LAUREL MD  US  20723-6005
Primary Place of Performance Congressional District:	03
Unique Entity Identifier (UEI):	FTMTDMBR29C7
Parent UEI:	GS4PNKTRNKL3
NSF Program(s):	MAGNETOSPHERIC PHYSICS
Primary Program Source:	01000809DB NSF RESEARCH & RELATED ACTIVIT app-0107  01000910DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s):	EGCH, 9196, 5295
Program Element Code(s):	575000
Award Agency Code:	4900
Fund Agency Code:	4900
Assistance Listing Number(s):	47.050

ABSTRACT

This is a three year research project to use data from the new SuperDARN radar at Wallops Island, as well as DMSP and Iridium satellite data to investigate and elicit the origins of what is known as Subauroral Polarization Streams (SAPS). The overarching science question is related to magnetosphere-ionosphere coupling, that is whether the ionosphere passively responds to the situation in the magnetosphere or whether the ionosphere should be considered as more tightly coupled to the magnetosphere so that it influences the whole magnetosphere-ionosphere response to the solar wind drivers. Specific science goals that will be addressed include 1) Quantifying the dawn-dusk asymmetry in the return flow including its variation with IMF clock angle; 2) Quantifying the asymmetry in intensity and latitude of particle precipitation and its relationship to: the return flow intensity, the Birkeland currents, and the IMF clock angle; 3) Determining whether inner magnetospheric convection including ring current physics can account for the observed distributions of flows and Birkeland currents or whether MHD physics without ion drift physics can account for the observed distribution of return flows.

The intellectual merit of this effort lies in significantly advancing our understanding of the storm-time Magnetosphere-Ionosphere system and the mid-latitude electrodynamics that occur during active times. This understanding is needed to advance the fundamental science understanding of geomagnetic storms but also has application to practical areas of importance such as communications and navigation for which strong ionospheric electric fields are of paramount concern. This project also continues an informal partnership between APL and the physics department at Augsburg College that consists in providing summer research opportunities for undergraduate students from Augsburg at APL via the JHU/APL Student Summer Internship program. M-I coupling during magnetic storms is one of the important physical processes that affect the upper atmospheric electrodynamics of the polar region. Thus, the research project will contribute to the larger research goals of the International Polar Year Program at NSF.

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