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Atmospheric OH Response to the 11-year Solar Cycle - Could the Gap Between Model and Observations Be Filled by New Satellite Data?No abstract available
Document ID
20150006054
Acquisition Source
Jet Propulsion Laboratory
Document Type
Presentation
External Source(s)
hdl:2014/43634
Authors
Wang, Shuhui (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Pongetti, Thomas J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Sander, Stanley P. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Li, King-Fai (California Inst. of Tech. Pasadena, CA, United States)
Yung, Yuk L. (California Inst. of Tech. Pasadena, CA, United States)
Liang, Mao-Chang (Academia Sinica Taipei, Taiwan, Province of China)
Livesey, Nathaniel J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Santee, Michelle L. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Harder, Jerald W. (Colorado Univ. Boulder, CO, United States)
Snow, Marty (Colorado Univ. Boulder, CO, United States)
Date Acquired
April 22, 2015
Publication Date
September 13, 2011
Subject Category
Solar Physics
Meeting Information
Meeting: EOS Aura Science Team Meeting
Location: Helsinki
Country: Finland
Start Date: September 13, 2011
End Date: September 15, 2011
Sponsors: NASA Goddard Space Flight Center
Distribution Limits
Public
Copyright
Other
Keywords
solar cycle signals
Fourier Transform Ultra-Violet Spectrometer

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IDRelationTitle20150005591See AlsoAtmospheric OH Response to the 11-year Solar Cycle and Implications for Ozone
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