🗊 Презентация Heat fluxes in the atmosphere

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Heat fluxes in the atmosphere, слайд №1 Heat fluxes in the atmosphere, слайд №2 Heat fluxes in the atmosphere, слайд №3 Heat fluxes in the atmosphere, слайд №4 Heat fluxes in the atmosphere, слайд №5 Heat fluxes in the atmosphere, слайд №6 Heat fluxes in the atmosphere, слайд №7 Heat fluxes in the atmosphere, слайд №8 Heat fluxes in the atmosphere, слайд №9 Heat fluxes in the atmosphere, слайд №10 Heat fluxes in the atmosphere, слайд №11 Heat fluxes in the atmosphere, слайд №12 Heat fluxes in the atmosphere, слайд №13 Heat fluxes in the atmosphere, слайд №14 Heat fluxes in the atmosphere, слайд №15 Heat fluxes in the atmosphere, слайд №16 Heat fluxes in the atmosphere, слайд №17

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Слайды и текст этой презентации


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Heat fluxes in the atmosphere Heat to the atmosphere comes mainly from the underlying surface. Processes responsible for the heat transfer are:
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Heat fluxes in the atmosphere Heat to the atmosphere comes mainly from the underlying surface. Processes responsible for the heat transfer are:

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Heat fluxes in the atmosphere, слайд №2
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Heat flux notion The quantity being transferred by the air parcels in a unit of time through a unit of area facing the transfer direction is called...
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Heat flux notion The quantity being transferred by the air parcels in a unit of time through a unit of area facing the transfer direction is called HEAT FLUX. There are convective heat flux and eddy heat flux. Convective heat flux, in turn, is divided into advective one (horizontal heat transfer) and real convective (vertical heat transfer). In meteorology, the horizontal heat flux is called advective flux (Qa), and the vertical one is called convective flux (Qc).

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Convective and advective heat fluxes
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Convective and advective heat fluxes

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Eddy heat flux Eddy heat flux is caused by wind velocity pulsation
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Eddy heat flux Eddy heat flux is caused by wind velocity pulsation

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Heat fluxes in the atmosphere, слайд №6
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Heat fluxes in the atmosphere, слайд №7
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Individual and local (partial) derivatives When an air parcel moves, its state parameters are not necessarily constant; they are function of...
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Individual and local (partial) derivatives When an air parcel moves, its state parameters are not necessarily constant; they are function of coordinates and time. For the moving parcel, the coordinates, in turn, are functions of time.

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Energy equation Temperature variation is of prime interest for meteorologists. It depends on heat influx. It can be determined on the base of the...
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Energy equation Temperature variation is of prime interest for meteorologists. It depends on heat influx. It can be determined on the base of the energy conservation equation. Heat influx:

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Heat fluxes in the atmosphere, слайд №10
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Heat fluxes in the atmosphere, слайд №11
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Heat fluxes in the atmosphere, слайд №12
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Heat fluxes in the atmosphere, слайд №13
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1. Non-periodical T variations Above boundary layer (in the free atm.) Small time intervals (about 24 h)  no heat influx  adiab. process Energy...
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1. Non-periodical T variations Above boundary layer (in the free atm.) Small time intervals (about 24 h)  no heat influx  adiab. process Energy equation:

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2. Periodical T variations Within the boundary layer (diurnal T variations) long time intervals  only vertical eddy heat influx Energy equation ( or...
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2. Periodical T variations Within the boundary layer (diurnal T variations) long time intervals  only vertical eddy heat influx Energy equation ( or equation of the conductivity of the atm.):

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3. Air mass moving over non-homogeneous surface Advection and eddy exchange are important Taking steady state process The process is called air mass...
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3. Air mass moving over non-homogeneous surface Advection and eddy exchange are important Taking steady state process The process is called air mass transformation Energy equation

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4. Annual T variation Most important role to Local, advective and convective derivatives  0 over a long period of time Energy equation
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4. Annual T variation Most important role to Local, advective and convective derivatives  0 over a long period of time Energy equation



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