SUBROUTINE mucorr(npts,pdeclin, plat, pmu, pfract,phaut,prad) IMPLICIT NONE c======================================================================= c c Calcul of equivalent solar angle and and fraction of day whithout c diurnal cycle. c c parmeters : c ----------- c c Input : c ------- c npts number of points c pdeclin solar declinaison c plat(npts) latitude c phaut hauteur typique de l'atmosphere c prad rayon planetaire c c Output : c -------- c pmu(npts) equivalent cosinus of the solar angle c pfract(npts) fractionnal day c c======================================================================= c----------------------------------------------------------------------- c c 0. Declarations : c ----------------- c Arguments : c ----------- INTEGER npts REAL plat(npts),pmu(npts), pfract(npts) REAL phaut,prad,pdeclin c c Local variables : c ----------------- INTEGER j REAL pi REAL z,cz,sz,tz,phi,cphi,sphi,tphi REAL ap,a,t,b REAL alph c----------------------------------------------------------------------- print*,'npts,pdeclin' print*,npts,pdeclin pi = 4. * atan(1.0) print*,'PI=',pi pi=2.*asin(1.) print*,'PI=B',pi z = pdeclin cz = cos (z) sz = sin (z) print*,'cz,sz',cz,sz DO 20 j = 1, npts phi = plat(j) cphi = cos(phi) if (cphi.le.1.e-9) cphi=1.e-9 sphi = sin(phi) tphi = sphi / cphi b = cphi * cz t = -tphi * sz / cz a = 1.0 - t*t ap = a IF(t.eq.0.) then t=0.5*pi ELSE IF (a.lt.0.) a = 0. t = sqrt(a) / t IF (t.lt.0.) then t = -atan (-t) + pi ELSE t = atan(t) ENDIF ENDIF pmu(j) = (sphi*sz*t) / pi + b*sin(t)/pi pfract(j) = t / pi IF (ap .lt.0.) then pmu(j) = sphi * sz pfract(j) = 1.0 ENDIF IF (pmu(j).le.0.0) pmu(j) = 0.0 pmu(j) = pmu(j) / pfract(j) IF (pmu(j).eq.0.) pfract(j) = 0. 20 CONTINUE c----------------------------------------------------------------------- c correction de rotondite: c ------------------------ alph=phaut/prad DO 30 j=1,npts c !!!!!! pmu(j)=sqrt(1224.*pmu(j)*pmu(j)+1.)/35. c $ (sqrt(alph*alph*pmu(j)*pmu(j)+2.*alph+1.)-alph*pmu(j)) 30 CONTINUE RETURN END