CCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3

Community Climate Model 3 (CCM3) is run on an idealized all land zonally symmetric planet (Terra Blanda) with no seasonality, no snow and fixed soil moisture to obtain a stationary time series effectively much longer than conventional runs with geography and seasons. The surface temperature field ge...

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Main Author: Mahajan, Salil
Other Authors: North, Gerald R.
Format: Others
Language:en_US
Published: Texas A&M University 2005
Subjects:
Online Access:http://hdl.handle.net/1969.1/1422
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spelling ndltd-tamu.edu-oai-repository.tamu.edu-1969.1-14222013-01-08T10:37:36ZCCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3Mahajan, SalilCCM3Terra Blandaall land planetidealizedzonally symmmetricsolar forcingssteady heat source forcingsfluctuation dissipation theoremextreme value statisticstemporal and spatial analysis of the surface temperature fieldlinearity of responseCommunity Climate Model 3 (CCM3) is run on an idealized all land zonally symmetric planet (Terra Blanda) with no seasonality, no snow and fixed soil moisture to obtain a stationary time series effectively much longer than conventional runs with geography and seasons. The surface temperature field generated is studied to analyze the spatial and temporal spectra, estimate the length scale and time scale of the model, and test the linearity of response to periodic and steady heat source forcings. The length scale of the model is found to be in the range of 1000-2000 km and the time scale is estimated to be 24 days for the global average surface temperature field. The response of the global average temperature is found to be fairly linear to periodic and the steady heat source forcings. The results obtained are compared with the results of a similar study that used CCM0. Fluctuation Dissipation theorem is also tested for applicability on CCM3. The response of the surface temperature field to a step function forcing is demonstrated to be very similar to the decay of naturally occurring anomalies, and the auto-correlation function. Return period of surface temperature anomalies is also studied. It is observed that the length of the data obtained from CCM3, though sufficient for analysis of first and second moments, is significantly deficient for return period analysis. An AR1 process is simulated to model the global averaged surface temperature of Terra Blanda 3 to assess the sampling error associated with short runs.Texas A&M UniversityNorth, Gerald R.2005-02-17T21:01:00Z2005-02-17T21:01:00Z2004-122005-02-17T21:01:00ZBookThesisElectronic Thesistext4392780 byteselectronicapplication/pdfborn digitalhttp://hdl.handle.net/1969.1/1422en_US
collection NDLTD
language en_US
format Others
sources NDLTD
topic CCM3
Terra Blanda
all land planet
idealized
zonally symmmetric
solar forcings
steady heat source forcings
fluctuation dissipation theorem
extreme value statistics
temporal and spatial analysis of the surface temperature field
linearity of response
spellingShingle CCM3
Terra Blanda
all land planet
idealized
zonally symmmetric
solar forcings
steady heat source forcings
fluctuation dissipation theorem
extreme value statistics
temporal and spatial analysis of the surface temperature field
linearity of response
Mahajan, Salil
CCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3
description Community Climate Model 3 (CCM3) is run on an idealized all land zonally symmetric planet (Terra Blanda) with no seasonality, no snow and fixed soil moisture to obtain a stationary time series effectively much longer than conventional runs with geography and seasons. The surface temperature field generated is studied to analyze the spatial and temporal spectra, estimate the length scale and time scale of the model, and test the linearity of response to periodic and steady heat source forcings. The length scale of the model is found to be in the range of 1000-2000 km and the time scale is estimated to be 24 days for the global average surface temperature field. The response of the global average temperature is found to be fairly linear to periodic and the steady heat source forcings. The results obtained are compared with the results of a similar study that used CCM0. Fluctuation Dissipation theorem is also tested for applicability on CCM3. The response of the surface temperature field to a step function forcing is demonstrated to be very similar to the decay of naturally occurring anomalies, and the auto-correlation function. Return period of surface temperature anomalies is also studied. It is observed that the length of the data obtained from CCM3, though sufficient for analysis of first and second moments, is significantly deficient for return period analysis. An AR1 process is simulated to model the global averaged surface temperature of Terra Blanda 3 to assess the sampling error associated with short runs.
author2 North, Gerald R.
author_facet North, Gerald R.
Mahajan, Salil
author Mahajan, Salil
author_sort Mahajan, Salil
title CCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3
title_short CCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3
title_full CCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3
title_fullStr CCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3
title_full_unstemmed CCM3 as applied to an idealized all land zonally symmetric planet, Terra Blanda 3
title_sort ccm3 as applied to an idealized all land zonally symmetric planet, terra blanda 3
publisher Texas A&M University
publishDate 2005
url http://hdl.handle.net/1969.1/1422
work_keys_str_mv AT mahajansalil ccm3asappliedtoanidealizedalllandzonallysymmetricplanetterrablanda3
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