A Quasi-Physical Dynamic Reduced Order Model for Thermospheric Mass Density via Hermitian Space-Dynamic Mode Decomposition-Reference-Cited by-同舟云学术

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A Quasi-Physical Dynamic Reduced Order Model for Thermospheric Mass Density via Hermitian Space-Dynamic Mode Decomposition

Published:2018-05 Issue:5 Volume:16 Page:569-588
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Mehta Piyush M.¹^ORCID,Linares Richard¹,Sutton Eric K.²^ORCID

Affiliation:

1. Department of Aerospace Engineering and Mechanics; University of Minnesota, Twin Cities; Minneapolis MN USA

2. Air Force Research Laboratory; Kirtland AFB; Albuquerque NM USA

Funder

Air Force's Office of Scientic Research

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2018SW001840/fullpdf

Reference23 articles.

1. Boyce , W. E. DiPrima , R. C. 2008 Elementary differential equations

2. Thermospheric mass density: A review;Emmert;Advances in Space Research,2015

3. Climatology of globally averaged thermospheric mass density;Emmert;Journal of Geophysical Research,2010

4. Erichson , N. B. Brunton , S. L. Kutz , J. 2017 Randomized dynamic mode decomposition https://doi.org/arXiv:1702.02912

5. Dynamics of the thermosphere;Forbes;Journal of the Meteorological Society of Japan,2007

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