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Grant: Research Tools and Instruments - Category 1 (<$150,000)

Queen's University

$85,716.00

Queen's solar radio telescope

FY 2006-07

Summary
The equipment in this proposal is necessary to improve the frequency and time accuracy  of the new solar radio telescope that we have built at Queen's with the support of CFI, OIT, Sun Microsystems, and Lucent. This telescope is the only one of its kind in the world and was built to study solar modes (stable oscillations) and their interaction with the terrestrial environment. Innovative features such as simultaneous 8-channel sampling, simultaneous noise and signal observation, and high and low gain channels, make it uniquely suited to observe the transition of low to high power output of the sun. We have built a unique modular receiver that is upgradable and serviceable by students and can be used for projects by 4th year Engineering students.     A major application is the study of dropped calls (cellular phone calls that are terminated unexpectedly for technical reasons).  A great amount of money and time are invested by wireless network providers to improve network quality of service, and dropped calls is one of the most important customer perceived problems that affect this quality.  The point is that a link has been clearly shown between dropped calls and solar activity. Understanding the correlation between these has broad implications for cell phone service providers and customers, and has the potential to affect the design of future wireless systems and the creation of a cell phone that is designed to overcome solar radio interference.  We have been promised data from both Roger's and Cingular's cellular networks to aid in this study.  Finding a solution to this problem will clearly benefit Canada's telecommunications industry.       In our search for the mechanism that causes a large fraction of the dropped call rate in cellular phone systems to be coherent with the solar modes we will need to observe inside the cellular bands and will need to replace the current YIG oscillator with a precision synthesizer to have sufficient frequency accuracy. We also need to add GPS timing to facilitate coordinated observations with those from the Bell Labs, Murray Hill, NJ, telescope, as originally planned.
Program
Research Tools and Instruments - Category 1 (<$150,000)
Location
Ontario, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data

As published

Application id
345686-2007
Name nom
Thomson, David
Department département
Mathematics and Statistics
Organization id
29
Institution établissement
Queen's University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2006
Competition year année de concours
2007
Award amount
85716
Program id
EQPEQ
Program name en
Research Tools and Instruments - Category 1 (<$150,000)
Program name fr
Outils et instruments de recherche - catégorie 1 (<150 000$)
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
335
Committee name en
Electromag. & Electr. Systems (H)
Committee name fr
Électromagn. et syst. électr. (H)
Area of application code
804
Area of application group en
Information and communication services
Area of application group fr
Services d'information et de télécommunications
Area of application en
Communication systems and services (planning, organization, services)
Area of application fr
Systèmes et services de communications (planification, organisation et services)
Research subject code
2507
Research subject group en
Electrical and electronic engineering
Research subject group fr
Génie électrique et électronique
Research subject en
Communications systems
Research subject fr
Systèmes de télécommunications
Partie
1
Nb partie
1
Application title
Queen's solar radio telescope
Keyword
NA
Application summary
The equipment in this proposal is necessary to improve the frequency and time accuracy  of the new solar radio telescope that we have built at Queen's with the support of CFI, OIT, Sun Microsystems, and Lucent. This telescope is the only one of its kind in the world and was built to study solar modes (stable oscillations) and their interaction with the terrestrial environment. Innovative features such as simultaneous 8-channel sampling, simultaneous noise and signal observation, and high and low gain channels, make it uniquely suited to observe the transition of low to high power output of the sun. We have built a unique modular receiver that is upgradable and serviceable by students and can be used for projects by 4th year Engineering students.     A major application is the study of dropped calls (cellular phone calls that are terminated unexpectedly for technical reasons).  A great amount of money and time are invested by wireless network providers to improve network quality of service, and dropped calls is one of the most important customer perceived problems that affect this quality.  The point is that a link has been clearly shown between dropped calls and solar activity. Understanding the correlation between these has broad implications for cell phone service providers and customers, and has the potential to affect the design of future wireless systems and the creation of a cell phone that is designed to overcome solar radio interference.  We have been promised data from both Roger's and Cingular's cellular networks to aid in this study.  Finding a solution to this problem will clearly benefit Canada's telecommunications industry.       In our search for the mechanism that causes a large fraction of the dropped call rate in cellular phone systems to be coherent with the solar modes we will need to observe inside the cellular bands and will need to replace the current YIG oscillator with a precision synthesizer to have sufficient frequency accuracy. We also need to add GPS timing to facilitate coordinated observations with those from the Bell Labs, Murray Hill, NJ, telescope, as originally planned.
Queen's University - $85,716 Grant (2006-07) | Canada Spends