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C $Header$ |
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C $Name$ |
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#include "DARWIN_OPTIONS.h" |
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CBOP |
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C !ROUTINE: DARWIN_SOLZ360 |
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C !INTERFACE: ====================================================== |
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SUBROUTINE darwin_solz360(Time,ylat, |
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O solz) |
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C !DESCRIPTION: |
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C Procedure name: DARWIN_SOLZ360 |
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C Function: find solar zenith angle for model calendar |
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C (360 day year) |
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c based on paltridge and parson |
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C cos(solz) = average cos(sol.zenith) during daylight |
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C Comments: swd, April 1998 |
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C following code by mick |
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C |
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C !USES: =========================================================== |
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IMPLICIT NONE |
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C !INPUT PARAMETERS: =============================================== |
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C time :: model time in seconds since Jan 1 (of start year) |
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C ylat :: latitude in degrees |
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_RL time, ylat |
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c INTEGER myThid |
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C !OUTPUT PARAMETERS: ============================================== |
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C delta :: solar zenith angle in degrees |
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_RL solz |
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C !FUNCTIONS: ====================================================== |
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C !LOCAL VARIABLES: ================================================ |
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_RL dayfrac, yday, delta, lat, sun1, dayhrs, cosz |
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CEOP |
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c find day (****NOTE for year starting in 1 Jan *****) |
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dayfrac = mod(Time, 360. _d 0*86400. _d 0) |
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& /(360. _d 0*86400. _d 0) !fraction of year |
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yday = 2.0 _d 0*3.1416 _d 0*dayfrac !convert to radians |
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delta = (0.006918 _d 0- (0.399912 _d 0*cos(yday)) !zenith angle |
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& +(0.070257 _d 0*sin(yday)) !(paltridge+platt) |
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& -(0.006758 _d 0*cos(2.0 _d 0*yday)) |
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& +(0.000907 _d 0*sin(2.0 _d 0*yday)) |
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& -(0.002697 _d 0*cos(3.0 _d 0*yday)) |
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& +(0.001480 _d 0*sin(3.0 _d 0*yday)) ) |
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lat = ylat/180. _d 0*3.1416 _d 0 |
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sun1 = -sin(delta)/cos(delta) * sin(lat)/cos(lat) |
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if (sun1.le.-0.999 _d 0) sun1=-0.999 _d 0 |
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if (sun1.ge. 0.999 _d 0) sun1= 0.999 _d 0 |
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dayhrs = abs(acos(sun1)) |
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cosz = ( sin(delta)*sin(lat)+ !average zenith angle |
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& (cos(delta)*cos(lat)*sin(dayhrs)/dayhrs) ) |
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if (cosz.le.0.005 _d 0) cosz=0.005 _d 0 |
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if (cosz.ge. 0.999 _d 0) cosz= 0.999 _d 0 |
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solz = acos(cosz)*180. _d 0/3.1416 _d 0 |
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c frac = dayhrs/3.1416 _d 0 !fraction of daylight in day |
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cc daily average photosynthetically active solar radiation just below surface |
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c fluxi = solar*(1.0 _d 0-albedo)*cosz*frac*par |
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cc |
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cc convert to sfac |
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c if (fluxi.gt.0.0 _d 0) sfac(j)=fluxi |
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cc very large for polar night |
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c if (fluxi.lt.0.00001 _d 0) sfac(j)=0.00001 _d 0 |
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return |
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end |
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c |
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C========================================================================== |