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The macroscopic temperature field is simulated using the temperature distribution function.
The whole temperature field can be reconstructed by using the FDM.
The temperature field for the entire specimen is also predicted.
Detailed temperature field information was obtained.
The temperature field determines the thermal strain in beryllium, which in turn changes the temperature field.
Steady state temperature field is assumed.
Evolution of temperature field and streamlines has been examined.
The flame shape and temperature field have been predicted.
On the basis of the model and the obtained surface temperature field, the interior temperature field is acquired.
In the temperature field, the meridional gradient changes its sign near the cloud-top level (∼70 km).
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Neutron, specific heat, and magnetization measurements produce a comprehensive temperature-field phase diagram.
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