Zobrazeno 1 - 5
of 5
pro vyhledávání: '"J. J. Tribbia"'
Autor:
P. H. Lauritzen, R. D. Nair, A. R. Herrington, P. Callaghan, S. Goldhaber, J. M. Dennis, J. T. Bacmeister, B. E. Eaton, C. M. Zarzycki, Mark A. Taylor, P. A. Ullrich, T. Dubos, A. Gettelman, R. B. Neale, B. Dobbins, K. A. Reed, C. Hannay, B. Medeiros, J. J. Benedict, J. J. Tribbia
Publikováno v:
Journal of Advances in Modeling Earth Systems, Vol 10, Iss 7, Pp 1537-1570 (2018)
Abstract It is the purpose of this paper to provide a comprehensive documentation of the new NCAR (National Center for Atmospheric Research) version of the spectral element (SE) dynamical core as part of the Community Earth System Model (CESM2.0) rel
Externí odkaz:
https://doaj.org/article/5ef923ff2c004d1eb752c501085d603b
Publikováno v:
Atmospheric Chemistry and Physics, Vol 11, Iss 16, Pp 8395-8413 (2011)
With the intent to gain further knowledge on the spectral structures and statistical regularities of surface atmospheric chemistry, the chemical gases (NO, NO2, NOx, CO, SO2, and O3) and aerosol (PM10) measured at 74 air quality monitoring stations o
Externí odkaz:
https://doaj.org/article/1be15957874546faac11beefd8106a97
Publikováno v:
Annales Geophysicae, Vol 29, Pp 221-227 (2011)
A new atmospheric dynamical core, named the High Order Method Modeling Environment (HOMME), has been recently included in the NCAR-Community Climate System Model version 4 (CCSM4). It is a petascale capable high-order element-based conservative dy
Externí odkaz:
https://doaj.org/article/d58e6f4eaf1d4c2b8a201051f2543f10
Publikováno v:
Nonlinear Processes in Geophysics, Vol 13, Iss 6, Pp 601-612 (2006)
The problem of data assimilation can be viewed as one of synchronizing two dynamical systems, one representing "truth" and the other representing "model", with a unidirectional flow of information between the two. Synchronization of truth and model d
Externí odkaz:
https://doaj.org/article/d9ccbb7940e64e14ae9ff576bf27cf90
Autor:
J. J. Tribbia, F. Baer
Publikováno v:
Monthly Weather Review. 105:1536-1539
A procedure is outlined which adjusts the initial conditions for any prediction model of a planetary fluid such that no motions of the fluid will evolve with high-frequency, gravity-type time scales despite the model's nonlinearity. Any model which c