200 likes | 1.1k Views
QUAL2K (p.19-20). 201110517 김세희. 4 TEMPERATURE MODEL . As in Figure 14, the heat balance takes into account heat transfers from adjacent elements, loads, withdrawals, the atmosphere, and the sediments. A heat balance can be written for element i as
E N D
QUAL2K (p.19-20) 201110517 김세희
4 TEMPERATURE MODEL • As in Figure 14, the heat balance takes into account heat transfers from adjacent elements, loads, withdrawals, the atmosphere, and the sediments. A heat balance can be written for element ias • where Ti = temperature in element i[oC], t = time [d], E’i= the bulk dispersion coefficient between elements iand i+ 1 [m3/d], Wh,i= the net heat load from point and non-point sources into element i[cal/d], ρw = the density of water [g/cm3], Cpw= the specific heat of water [cal/(g oC)], Ja,i= the air-water heat flux [cal/(cm2 d)], and Js,i= the sediment-water heat flux [cal/(cm2 d)].
The bulk dispersion coefficient is computed as • Note that two types of boundary condition are used at the river’s downstream terminus: (1) a zero dispersion condition (natural boundary condition) and (2) a prescribed downstream boundary condition (Dirichlet boundary condition). The choice between these options is made on the Downstream Worksheet. • The net heat load from sources is computed as (recall Eq. 2) • where Tps,i,jis the temperature of the jth point source for element i[oC], and Tnps,i,jis the temperature of the jth non-point source temperature for element i[oC].
4.1 Surface Heat Flux • As depicted in Figure 15, surface heat exchange is modeled as a combination of five processes: • where I(0) = net solar shortwave radiation at the water surface, Jan = net atmospheric longwave radiation, Jbr= longwave back radiation from the water, Jc= conduction, and Je = evaporation. All fluxes are expressed as cal/cm2/d.
4.1.1 Solar Radiation • The model computes the amount of solar radiation entering the water at a particular latitude Lat (Lat ) and longitude (Llm) on the earth’s surface. This quantity is a function of the radiation at the top of the earth’s atmosphere which is attenuated by atmospheric transmission, cloud cover, reflection, and shade, • Extraterrestrial atmospheric cloud reflection shading • Radiation attenuation attenuation
where I(0) = solar radiation at the water surface [cal/cm2/d], I0 = extraterrestrial radiation (i.e., at the top of the earth’s atmosphere) [cal/cm2/d], at = atmospheric attenuation, ac = cloud attenuation, Rs = albedo (fraction reflected), and Sf= effective shade (fraction blocked by vegetation and topography). • Extraterrestrial radiation. The extraterrestrial radiation is computed as (TVA 1972)