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Grant: Discovery Grants Program - Individual

University of Alberta

$122,000.00

The Role of Alfven Wave Energy Transport in Geospace Dynamics

FY 2022-23

Summary
Space plasma physics in the solar system is a major focus for current and future national and international space agency missions. This research focuses on the fundamental processes active in solar and planetary plasma environments, a plasma being a hot ionised gas, strongly influenced by magnetic fields. The same processes are active in high energy plasma astrophysical systems, in magnetic fusion reactors, and their affects are felt on Earth and by human explorers in the solar system through the impacts of space weather. At the core of this research is are numerous important outstanding questions: whether this be the how energy is extracted from magnetic fields through a fundamental process known as magnetic reconnection, why the outer atmosphere of the sun (the solar coronal) is millions of degrees hotter than the 6000 degrees at the surface, how the solar wind is accelerated, or how magnetic storms affect our planet and result in the acceleration of particles to relativistic speeds! Such processes are important throughout the astrophysical universe, but only in the solar system can spacecraft collect the data needed to advance scientific understanding. The operation of a fleet international satellites around the Earth and in the solar system presents a unique opportunity for discovery. This is heralding a golden age for space research, and exploiting this opportunity is the focus of the Discovery Grant research and training proposed here.Our proposed research focuses on the impacts of Alfven waves in controlling geospace dynamics. Alfven waves are low-frequency waves whose energy transport and signals are guided by the magnetic field. Despite an increasing recognition that they are pervasive in these plasma systems, the potential that Alfven waves may control a number of energetically significant processes is only now beginning to be explored in detail. This is especially true at Earth in relation to radiation belt dynamics, and perhaps also to the dynamics of electrical current systems, and coupling between the ionised and neutral atmosphere, and perhaps even to climate. Addressing the role of Alfven waves in these processes are the specific research topics to be addressed in this proposal. Significantly, and according to a US National Academies report in 2008, space weather also represents a potential $2 Trillion USD threat to 21st century technological infrastructure in the US alone, including impacts on the electrical power grid, satellite systems, and communications networks. As a result, the research and training proposed here is also very timely since it aligns perfectly with an increasingly important need to understand, forecast, and mitigate the impacts arising from space weather. This ensures that the fundamental science discoveries arising from the proposed research will additionally have high profile applications, with national and indeed international importance.
Program
Discovery Grants Program - Individual
Location
Alberta, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data

As published

Application id
RGPIN-2018-06006
Name nom
Mann, Ian
Department département
Physics - Physics
Organization id
9
Institution établissement
University of Alberta
Province en
Alberta
Province fr
Alberta
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2022
Competition year année de concours
2018
Award amount
122000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
DISCOVERY RESEARCH
Group fr
RECHERCHE AXÉE SUR LA DÉCOUVERTE
Committee code
1505
Committee name en
Physics
Committee name fr
Physique
Area of application code
1204
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Space and astronomy
Area of application fr
Sciences spatiales et astronomie
Research subject code
3250
Research subject group en
Space science
Research subject group fr
Recherche spatiale
Research subject en
Space science
Research subject fr
Recherche spatiale
Installment
inst:5;6
Partie
2
Nb partie
6
Application title
The Role of Alfven Wave Energy Transport in Geospace Dynamics
Application summary
Space plasma physics in the solar system is a major focus for current and future national and international space agency missions. This research focuses on the fundamental processes active in solar and planetary plasma environments, a plasma being a hot ionised gas, strongly influenced by magnetic fields. The same processes are active in high energy plasma astrophysical systems, in magnetic fusion reactors, and their affects are felt on Earth and by human explorers in the solar system through the impacts of space weather. At the core of this research is are numerous important outstanding questions: whether this be the how energy is extracted from magnetic fields through a fundamental process known as magnetic reconnection, why the outer atmosphere of the sun (the solar coronal) is millions of degrees hotter than the 6000 degrees at the surface, how the solar wind is accelerated, or how magnetic storms affect our planet and result in the acceleration of particles to relativistic speeds! Such processes are important throughout the astrophysical universe, but only in the solar system can spacecraft collect the data needed to advance scientific understanding. The operation of a fleet international satellites around the Earth and in the solar system presents a unique opportunity for discovery. This is heralding a golden age for space research, and exploiting this opportunity is the focus of the Discovery Grant research and training proposed here.Our proposed research focuses on the impacts of Alfven waves in controlling geospace dynamics. Alfven waves are low-frequency waves whose energy transport and signals are guided by the magnetic field. Despite an increasing recognition that they are pervasive in these plasma systems, the potential that Alfven waves may control a number of energetically significant processes is only now beginning to be explored in detail. This is especially true at Earth in relation to radiation belt dynamics, and perhaps also to the dynamics of electrical current systems, and coupling between the ionised and neutral atmosphere, and perhaps even to climate. Addressing the role of Alfven waves in these processes are the specific research topics to be addressed in this proposal. Significantly, and according to a US National Academies report in 2008, space weather also represents a potential $2 Trillion USD threat to 21st century technological infrastructure in the US alone, including impacts on the electrical power grid, satellite systems, and communications networks. As a result, the research and training proposed here is also very timely since it aligns perfectly with an increasingly important need to understand, forecast, and mitigate the impacts arising from space weather. This ensures that the fundamental science discoveries arising from the proposed research will additionally have high profile applications, with national and indeed international importance.