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@ARTICLE{Tratt:844807,
      author       = {Tratt, David M. and Hackwell, John A. and Valant-Spaight,
                      Bonnie L. and Walterscheid, Richard L. and Gelinas, Lynette
                      J. and Hecht, James H. and Swenson, Charles M. and Lampen,
                      Caleb P. and Alexander, M. Joan and Hoffmann, Lars and
                      Nolan, David S. and Miller, Steven D. and Hall, Jeffrey L.
                      and Atlas, Robert and Marks, Frank D. and Partain, Philip
                      T.},
      title        = {{GHOST}: {A} {S}atellite {M}ission {C}oncept for
                      {P}ersistent {M}onitoring of {S}tratospheric {G}ravity
                      {W}aves {I}nduced by {S}evere {S}torms},
      journal      = {Bulletin of the American Meteorological Society},
      volume       = {99},
      issn         = {1520-0477},
      address      = {Boston, Mass.},
      publisher    = {ASM},
      reportid     = {FZJ-2018-02181},
      pages        = {1813–1828},
      year         = {2018},
      abstract     = {The prediction of tropical cyclone rapid intensification is
                      one of the most pressing unsolved problems in hurricane
                      forecasting. The signatures of gravity waves launched by
                      strong convective updrafts are often clearly seen in airglow
                      and carbon dioxide thermal emission spectra under favorable
                      atmospheric conditions. By continuously monitoring the
                      Atlantic hurricane belt from the main development region to
                      the vulnerable sections of the continental U.S. at high
                      cadence it will be possible to investigate the utility of
                      storm-induced gravity wave observations for the diagnosis of
                      impending storm intensification. Such a capability would
                      also enable significant improvements in our ability to
                      characterize the 3D, transient behavior of upper atmospheric
                      gravity waves, and point the way to future observing
                      strategies that could mitigate the risk to human life due to
                      severe storms. This paper describes a new mission concept
                      involving a mid-infrared imager hosted aboard a
                      geostationary satellite positioned at approximately 80°W
                      longitude. The sensor’s 3-km pixel size ensures that
                      gravity wave horizontal structure is adequately resolved,
                      while a 30-s refresh rate enables improved definition of the
                      dynamic intensification process. In this way the transient
                      development of gravity wave perturbations caused by both
                      convective and cyclonic storms may be discerned in near
                      realtime.},
      cin          = {JSC},
      ddc          = {550},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {511 - Computational Science and Mathematical Methods
                      (POF3-511)},
      pid          = {G:(DE-HGF)POF3-511},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000448508300008},
      doi          = {10.1175/BAMS-D-17-0064.1},
      url          = {https://juser.fz-juelich.de/record/844807},
}