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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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 |
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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 |
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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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1716502789219155968 |