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| Hauptseite > Publikationsdatenbank > GHOST: A Satellite Mission Concept for Persistent Monitoring of Stratospheric Gravity Waves Induced by Severe Storms > print |
| Hauptseite > Publikationsdatenbank > GHOST: A Satellite Mission Concept for Persistent Monitoring of Stratospheric Gravity Waves Induced by Severe Storms > print |
| 001 | 844807 | ||
| 005 | 20210129233114.0 | ||
| 024 | 7 | _ | |a 10.1175/BAMS-D-17-0064.1 |2 doi |
| 024 | 7 | _ | |a 0003-0007 |2 ISSN |
| 024 | 7 | _ | |a 1520-0477 |2 ISSN |
| 024 | 7 | _ | |a 2128/19819 |2 Handle |
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| 037 | _ | _ | |a FZJ-2018-02181 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 550 |
| 100 | 1 | _ | |a Tratt, David M. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a GHOST: A Satellite Mission Concept for Persistent Monitoring of Stratospheric Gravity Waves Induced by Severe Storms |
| 260 | _ | _ | |a Boston, Mass. |c 2018 |b ASM |
| 336 | 7 | _ | |a article |2 DRIVER |
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| 520 | _ | _ | |a 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. |
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| 700 | 1 | _ | |a Hackwell, John A. |0 P:(DE-HGF)0 |b 1 |
| 700 | 1 | _ | |a Valant-Spaight, Bonnie L. |0 P:(DE-HGF)0 |b 2 |
| 700 | 1 | _ | |a Walterscheid, Richard L. |0 P:(DE-HGF)0 |b 3 |
| 700 | 1 | _ | |a Gelinas, Lynette J. |0 P:(DE-HGF)0 |b 4 |
| 700 | 1 | _ | |a Hecht, James H. |0 P:(DE-HGF)0 |b 5 |
| 700 | 1 | _ | |a Swenson, Charles M. |0 P:(DE-HGF)0 |b 6 |
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| 700 | 1 | _ | |a Nolan, David S. |0 P:(DE-HGF)0 |b 10 |
| 700 | 1 | _ | |a Miller, Steven D. |0 P:(DE-HGF)0 |b 11 |
| 700 | 1 | _ | |a Hall, Jeffrey L. |0 P:(DE-HGF)0 |b 12 |
| 700 | 1 | _ | |a Atlas, Robert |0 P:(DE-HGF)0 |b 13 |
| 700 | 1 | _ | |a Marks, Frank D. |0 P:(DE-HGF)0 |b 14 |
| 700 | 1 | _ | |a Partain, Philip T. |0 P:(DE-HGF)0 |b 15 |
| 773 | _ | _ | |a 10.1175/BAMS-D-17-0064.1 |g p. BAMS-D-17-0064.1 |0 PERI:(DE-600)2029396-3 |p 1813–1828 |t Bulletin of the American Meteorological Society |v 99 |y 2018 |x 1520-0477 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/844807/files/bams-d-17-0064.1.pdf |y Published on 2018-10-09. Available in OpenAccess from 2019-04-09. |
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