Grant: Discovery Grants Program - Individual
York University
$36,100.00
To further the understanding of upper atmospheric dynamics using existing and future satellite observations
EF 2018-19
Résumé
This application builds on ""the old"" to create ""the new"". In 1991, an instrument of my conception called ""The Wind Imaging Interferometer"" (WINDII), was launched on NASA's Upper Atmospheric Research Satellite, a field-widened phase-stepping Michelson interferometer. It was built in Canadian industry, in collaboration with France. Funding was from the Canadian Space Agency with the scientific analysis supported by NSERC. Its objective was to measure winds and airglow emission rates of the atmosphere between 85 and 300 km above the Earth's surface. WINDII had a mass of 45 kg, on a 7000 kg satellite, whose size made possible exceptional performance. WINDII operated until 2003, obtaining unique results from some 23 million images of the upper atmosphere, producing 149 refereed publications of which the applicant was the lead author on 28 and co-author on 74. Most recent were by Dhadly et al. (2017,a,b) on winds in the polar atmosphere incorporating ground-based and satellite results in which the WINDII data provided winds not accessible to any other instrument. WINDII has provided new knowledge of the dynamics of the upper atmosphere, through the study of its constituents, and its migrating and non-migrating tides about which little was known before WINDII, and further contributions are to come. In December, 2017, a NASA instrument called MIGHTI will be launched that will provide the first results comparable to WINDII, some 26 years later, revealing the atmospheric changes over that time. * Following the success of WINDII, other approaches were considered for future Canadian missions. One supported by the CSA was adding Spatial Heterodyne Spectroscopy (SHS) to the WINDII approach. With this, the phase stepping is accomplished with no moving components and with all phase elements observed simultaneously rather than sequentially. The first version of this was for the measurement of water vapour in the atmosphere and this was flown on a high-altitude balloon and has just been flown on the NASA ER-2 aircraft. * As a result we were approached by Dr. Martin Kaufmann of the Juelich Institute of Energy and Climate Reseach in Germany in 2015 for a collaboration on upper atmospheric temperature, including atomic oxygen concentration, and an SHS instrument was jointly designed with their funding. Called AtmoSHINE, it was built in Germany but with no flight opportunity. Through York University contacts with the Beijing Aerospace Control Centre space was found on a Chinese satellite and launch is planned for June, 2018. *Thus the proposed work will combine ""the new"" with ""the old"" in conducting the following program. *1. Continued analysis of WINDII results, extending the current knowledge for the benefit of Canadians.*2. Analysis of AtmoSHINE results on large scale waves in temperature and atomic oxygen concentrations.*3. Comparison of WINDII results with those from MIGHTI, taken 26 years later, to assess atmospheric change.
Programme
Discovery Grants Program - Individual
Bénéficiaire
Emplacement
Ontario, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data
Tel que publié
Application id
RGPIN-2018-05940
Name nom
Shepherd, Gordon
Department département
Earth and Space Science and Engineering
Organization id
38
Institution établissement
York University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2018
Competition year année de concours
2018
Award amount
36100
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à 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
3252
Research subject group en
Space science
Research subject group fr
Recherche spatiale
Research subject en
Upper atmosphere
Research subject fr
Haute atmosphère
Partie
1
Nb partie
5
Application title
To further the understanding of upper atmospheric dynamics using existing and future satellite observations
Keyword
NSERC
Application summary
This application builds on ""the old"" to create ""the new"". In 1991, an instrument of my conception called ""The Wind Imaging Interferometer"" (WINDII), was launched on NASA's Upper Atmospheric Research Satellite, a field-widened phase-stepping Michelson interferometer. It was built in Canadian industry, in collaboration with France. Funding was from the Canadian Space Agency with the scientific analysis supported by NSERC. Its objective was to measure winds and airglow emission rates of the atmosphere between 85 and 300 km above the Earth's surface. WINDII had a mass of 45 kg, on a 7000 kg satellite, whose size made possible exceptional performance. WINDII operated until 2003, obtaining unique results from some 23 million images of the upper atmosphere, producing 149 refereed publications of which the applicant was the lead author on 28 and co-author on 74. Most recent were by Dhadly et al. (2017,a,b) on winds in the polar atmosphere incorporating ground-based and satellite results in which the WINDII data provided winds not accessible to any other instrument. WINDII has provided new knowledge of the dynamics of the upper atmosphere, through the study of its constituents, and its migrating and non-migrating tides about which little was known before WINDII, and further contributions are to come. In December, 2017, a NASA instrument called MIGHTI will be launched that will provide the first results comparable to WINDII, some 26 years later, revealing the atmospheric changes over that time. * Following the success of WINDII, other approaches were considered for future Canadian missions. One supported by the CSA was adding Spatial Heterodyne Spectroscopy (SHS) to the WINDII approach. With this, the phase stepping is accomplished with no moving components and with all phase elements observed simultaneously rather than sequentially. The first version of this was for the measurement of water vapour in the atmosphere and this was flown on a high-altitude balloon and has just been flown on the NASA ER-2 aircraft. * As a result we were approached by Dr. Martin Kaufmann of the Juelich Institute of Energy and Climate Reseach in Germany in 2015 for a collaboration on upper atmospheric temperature, including atomic oxygen concentration, and an SHS instrument was jointly designed with their funding. Called AtmoSHINE, it was built in Germany but with no flight opportunity. Through York University contacts with the Beijing Aerospace Control Centre space was found on a Chinese satellite and launch is planned for June, 2018. *Thus the proposed work will combine ""the new"" with ""the old"" in conducting the following program. *1. Continued analysis of WINDII results, extending the current knowledge for the benefit of Canadians.*2. Analysis of AtmoSHINE results on large scale waves in temperature and atomic oxygen concentrations.*3. Comparison of WINDII results with those from MIGHTI, taken 26 years later, to assess atmospheric change.