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Award Abstract #0520546
Long Term Observations of the Arctic Upper Atmosphere using the Kodiak SuperDARN Radar


NSF Org: ARC
Arctic Sciences Division
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Initial Amendment Date: March 14, 2006
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Latest Amendment Date: April 9, 2009
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Award Number: 0520546
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Award Instrument: Continuing grant
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Program Manager: Renee D. Crain
ARC Arctic Sciences Division
OPP Office of Polar Programs
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Start Date: March 15, 2006
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Expires: February 28, 2010 (Estimated)
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Awarded Amount to Date: $793607
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Investigator(s): William Bristow bill.bristow@gi.alaska.edu (Principal Investigator)
John Hughes (Co-Principal Investigator)
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Sponsor: University of Alaska Fairbanks Campus
Adm Svcs Ctr Rm 109
Fairbanks, AK 99709 907/474-7314
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NSF Program(s): ARCTIC RESRCH SUPPRT & LOGISTI,
ANTARCTIC AERONOMY & ASTROPHYS,
UPPER ATMOSPHERIC FACILITIES
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Field Application(s): 0311000 Polar Programs-Related
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Program Reference Code(s): OTHR, 9150, 4444, 1079, 0000
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Program Element Code(s): 5205, 5115, 4202

ABSTRACT

The overall goal of this project is to continue the operations of the Kodiak SuperDARN Radar.

The Super Dual Auroral Radar Network, or SuperDARN, is an international collaborative

experiment for observations of plasma motions in Earth's upper atmosphere. By observing ionospheric plasma motions, a multitude of geophysical processes can be studied. These

processes range from E-region plasma instabilities, to the relationships between auroral

luminosity and electric fields, to the global-scale convective response to changes in the solar

wind and interplanetary magnetic field. Each of these areas of study contributes to the overall

goals of space physics: developing an understanding of the coupling of energy from the solar

wind into Earth's upper atmosphere and its effects on man or manmade systems. The Kodiak radar is particularly well suited for studies of he general areas to be addressed are convection observations, substorm processes, dayside transients, reconnection features at the cusp, mesospheric winds observed in meteor scatter, gravity waves, and thermosphere-ionosphere interactions, and these will be supported by this award.

The SuperDARN network comprises nine radars in the northern hemisphere, and seven radars in

the southern hemisphere, each operated independently by the member institutions, and supported

by the national agencies in their countries of residence. As is the nature of such networks, data from the SuperDARN network are used in such a wide variety of studies by such a wide range of scientists that it is prohibitive to produce a comprehensive list of the topics.


PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

(Showing: 1 - 4 of 4).

Bristow, W.  "Statistics of velocity fluctuations observed by SuperDARN under steady interplanetary magnetic field conditions,"  JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,  v.113,  2008,   

Bristow, WA; Jensen, P.  "A superposed epoch study of SuperDARN convection observations during substorms,"  JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,  v.112,  2007,   

Chisham, G; Lester, M; Milan, SE; Freeman, MP; Bristow, WA; Grocott, A; McWilliams, KA; Ruohoniemi, JM; Yeoman, TK; Dyson, PL; Greenwald, RA; Kikuchi, T; Pinnock, M; Rash, JPS; Sato, N; Sofko, GJ; Villain, JP; Walker, ADM.  "A decade of the Super Dual Auroral Radar Network (SuperDARN): scientific achievements, new techniques and future directions,"  SURVEYS IN GEOPHYSICS,  v.28,  2007,  p. 33 - 109.  

Kosch, MJ; Pedersen, T; Mishin, E; Oyama, S; Hughes, J; Senior, A; Watkins, B; Bristow, B.  "Coordinated optical and radar observations of ionospheric pumping for a frequency pass through the second electron gyroharmonic at HAARP,"  JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,  v.112,  2007,   


(Showing: 1 - 4 of 4).

 

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Last Updated:April 2, 2007