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fc4b33f934
git-svn-id: svn+ssh://svn.code.sf.net/p/wsjt/wsjt/branches/wsjtx@6575 ab8295b8-cf94-4d9e-aec4-7959e3be5d79
80 lines
2.0 KiB
Fortran
80 lines
2.0 KiB
Fortran
subroutine sync9w(ss,nzhsym,lag1,lag2,ia,ib,ccfred,ccfblue,ipkbest,lagpk,nadd)
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include 'constants.f90'
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real ss(184,NSMAX)
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real ss1(184),ss1save(184)
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real ccfred(NSMAX)
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real ccfblue(-9:18)
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real sa(NSMAX),sb(NSMAX)
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include 'jt9sync.f90'
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! Smooth the symbol spectra (by an amount consistent with measured width??)
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do j=1,nzhsym
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sa=ss(j,1:NSMAX)
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call smo(sa,NSMAX,sb,nadd)
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call smo(sb,NSMAX,sa,nadd)
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ss(j,1:NSMAX)=sa
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enddo
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ipk=0
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ipkbest=0
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sbest=0.
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ccfred=0.
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df=12000.0/16384.0
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do i=ia,ib !Loop over specified freq range
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ss1=ss(1:184,i) !Symbol amplitudes at this freq
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call pctile(ss1,nzhsym,50,xmed) !Median level at this freq
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ss1=ss1/xmed - 1.0
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smax=0. !Find DT in specified range
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do lag=lag1,lag2
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sum1=0.
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nsum=nzhsym
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do j=1,16 !Sum over 16 sync symbols
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k=ii2(j) + lag
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if(k.ge.1 .and. k.le.nzhsym) then
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sum1=sum1 + ss1(k)
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nsum=nsum-1
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endif
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enddo
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if(sum1.gt.smax) then
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smax=sum1
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ipk=i
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endif
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enddo
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ccfred(i)=smax !Best at this freq, over all lags
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if(smax.gt.sbest) then
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sbest=smax
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ipkbest=ipk
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ss1save=ss1
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endif
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enddo
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call pctile(ccfred(ia),ib-ia+1,50,xmed)
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if(xmed.le.0.0) xmed=1.0
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ccfred=ccfred/xmed
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ss1=ss1save
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smax=0. !Find DT in specified range
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do lag=lag1,lag2
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sum1=0.
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nsum=nzhsym
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do j=1,16 !Sum over 16 sync symbols
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k=ii2(j) + lag
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if(k.ge.1 .and. k.le.nzhsym) then
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sum1=sum1 + ss1(k)
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nsum=nsum-1
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endif
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enddo
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ccfblue(lag)=sum1
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if(sum1.gt.smax) then
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smax=sum1
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lagpk=lag
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endif
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enddo
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return
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end subroutine sync9w
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