WSJT-X/libm65/specjtms.f90
Joe Taylor ad7f10843e Further mods toward implementing JT8 modes.
git-svn-id: svn+ssh://svn.code.sf.net/p/wsjt/wsjt/branches/wsjtx@2596 ab8295b8-cf94-4d9e-aec4-7959e3be5d79
2012-09-25 16:04:38 +00:00

107 lines
2.1 KiB
Fortran

subroutine specjtms(k,px,pxsmo,spk0,f0)
! Compute noise level and 2D spectra, for GUI display.
parameter (NSMAX=30*48000)
parameter (MAXFFT=8192)
integer*2 id
real x(MAXFFT)
complex cx(MAXFFT),cx2(MAXFFT)
logical first
common/mscom/id(1440000),s1(215),s2(215),kin,ndiskdat,kline,nutc
common/jt8com/nn(1800*12000),ss(184,32768),savg(32768)
data first/.true./
save
if(first) then
pi=4.0*atan(1.0)
twopi=2.0*pi
kstep=2048
first=.false.
sqsmo=0.
endif
if(k.lt.kstep .or. k.gt.NSMAX) return
t=k/48000.0
nfft=4096
df=48000.0/nfft
nh=nfft/2
ib=k
ia=k-kstep+1
i0=k-nfft+1
sq=0.
do i=ia,ib
d=id(i)
sq=sq + d*d
enddo
sq=sq/2048.0
sqsmo=0.95*sqsmo + 0.05*sq
rms=sqrt(sq)
px=db(sq) - 23.0
pxsmo=db(sqsmo) - 23.0
if(i0.gt.0) then
do i=i0,ia-1
d=id(i)
sq=sq + d*d
enddo
endif
sq0=sq
! write(13,1010) t,rms,sq,px,pxsmo
!1010 format(5f12.3)
if(k.lt.nfft) return
x(1:nfft)=id(i0:ib)
fac=0.002/nfft
cx=fac*x
call four2a(cx,nfft,1,-1,1) !Forward c2c FFT
iz=nint(2500.0/df)
do i=1,iz !Save spectrum for plot
s1(i)=real(cx(i+1))**2 + aimag(cx(i+1))**2
enddo
cx(1)=0.5*cx(1)
cx(nh+2:nfft)=0.
call four2a(cx,nfft,1,1,1) !Inverse c2c FFT
cx2(1:nfft)=cx(1:nfft)*cx(1:nfft)
cx2(nfft+1:)=0.0
nfft=8192
df=48000.0/nfft
call four2a(cx2,nfft,1,-1,1) !Forward c2c FFT of cx2
! j0=nint(2.0*1428.57/df)
j0=nint(2.0*1500.0/df)
ja=j0-107
jb=j0+107
do j=ja,jb
s2(j-ja+1)=1.e-4*(real(cx2(j))**2 + aimag(cx2(j))**2)
enddo
spk0=0.
fac=(5e8/sq0)**2
s2=fac*s2
do j=1,215
if(s2(j).gt.spk0) then
spk0=s2(j)
f=(j+ja-1)*df
f0=0.5*(f-3000.0)
phi0=0.5*atan2(aimag(cx2(j)),real(cx2(j)))
endif
enddo
spk0=0.5*db(spk0) - 7.0
kline=k/2048
! write(14,3001) k/2048,spk0,f0,phi0
!3001 format(i8,3f12.3)
! call flush(14)
return
end subroutine specjtms