WSJT-X/spec.f90
Joe Taylor c80ba1b2ed Split Audio.f90 into separate routines
git-svn-id: svn+ssh://svn.code.sf.net/p/wsjt/wsjt/WSJT/trunk@10 ab8295b8-cf94-4d9e-aec4-7959e3be5d79
2005-12-23 17:07:54 +00:00

214 lines
5.5 KiB
Fortran

!---------------------------------------------------- End Module Audio1
!---------------------------------------------------- spec
subroutine spec(brightness,contrast,logmap,ngain,nspeed,a)
! Called by SpecJT in its TopLevel Python code.
! Probably should use the "!f2py intent(...)" structure here.
! Input:
integer brightness,contrast !Display parameters
integer ngain !Digital gain for input audio
integer nspeed !Scrolling speed index
! Output:
integer*2 a(225000) !Pixel values for 750 x 300 array
real psa(750) !Grand average spectrum
real ref(750) !Ref spect: smoothed ave of lower half
real birdie(750) !Spec (with birdies) for plot, in dB
real variance(750) !Variance in each spectral channel
real a0(225000) !Save the last 300 spectra
integer*2 idat(11025) !Sound data, read from file
integer nstep(5)
integer b0,c0
real x(4096) !Data for FFT
complex c(0:2048) !Complex spectrum
real ss(1024) !Bottom half of power spectrum
logical first
include 'gcom1.f90'
include 'gcom2.f90'
include 'gcom3.f90'
include 'gcom4.f90'
data jz/0/ !Number of spectral lines available
data nstep/15,10,5,2,1/ !Integration limits
data first/.true./
equivalence (x,c)
save
if(first) then
call zero(ss,nq)
istep=2205
nfft=4096
nq=nfft/4
df=11025.0/nfft
fac=2.0/10000.
nsum=0
iread=0
cversion='5.5.0 '
first=.false.
b0=-999
c0=-999
logmap0=-999
nspeed0=-999
nx=0
ncall=0
jza=0
rms=0.
endif
nmode=1
if(mode(1:4).eq.'JT65') nmode=2
if(mode.eq.'Echo') nmode=3
if(mode.eq.'JT6M') nmode=4
nlines=0
newdat=0
npts=iwrite-iread
if(ndiskdat.eq.1) then
npts=jzc/2048
npts=2048*npts
kread=0
if(nspeed.ge.6) then
call hscroll(a,nx)
nx=0
endif
endif
if(npts.lt.0) npts=npts+nmax
if(npts.lt.nfft) go to 900 !Not enough data available
10 continue
if(ndiskdat.eq.1) then
! Data read from disk
k=kread
do i=1,nfft
k=k+1
x(i)=0.4*d2c(k)
enddo
kread=kread+istep !Update pointer
else
! Real-time data
dgain=2.0*10.0**(0.005*ngain)
k=iread
do i=1,nfft
k=k+1
if(k.gt.nmax) k=k-nmax
x(i)=0.5*dgain*y1(k)
enddo
iread=iread+istep !Update pointer
if(iread.gt.nmax) iread=iread-nmax
endif
sum=0. !Get ave, rms of data
do i=1,nfft
sum=sum+x(i)
enddo
ave=sum/nfft
sq=0.
do i=1,nfft
d=x(i)-ave
sq=sq+d*d
x(i)=fac*d
enddo
rms1=sqrt(sq/nfft)
if(rms.eq.0) rms=rms1
rms=0.25*rms1 + 0.75*rms
if(ndiskdat.eq.0) then
level=0 !Compute S-meter level
if(rms.gt.0.0) then !Scale 0-100, steps = 0.4 dB
dB=20.0*log10(rms/800.0)
level=50 + 2.5*dB
if(level.lt.0) level=0
if(level.gt.100) level=100
endif
endif
if(nspeed.ge.6) then
call horizspec(x,brightness,contrast,a)
ncall=Mod(ncall+1,5)
if(ncall.eq.1 .or. nspeed.eq.7) newdat=1
if(ndiskdat.eq.1) then
npts=jzc-kread
else
npts=iwrite-iread
if(npts.lt.0) npts=npts+nmax
endif
if(npts.ge.4096) go to 10
go to 900
endif
call xfft(x,nfft)
do i=1,nq !Accumulate power spectrum
ss(i)=ss(i) + real(c(i))**2 + imag(c(i))**2
enddo
nsum=nsum+1
if(nsum.ge.nstep(nspeed)) then !Integrate for specified time
nlines=nlines+1
do i=225000,751,-1 !Move spectra up one row
a0(i)=a0(i-750) ! (will be "down" on display)
enddo
if(ndiskdat.eq.1 .and. nlines.eq.1) then
do i=1,750
a0(i)=255
enddo
do i=225000,751,-1
a0(i)=a0(i-750)
enddo
endif
if(nflat.gt.0) call flat2(ss,1024,nsum)
do i=1,750 !Insert new data in top row
j=i+182 ! ?? was 186 ??
a0(i)=5*ss(j)/nsum
xdb=-40.
if(a0(i).gt.0.) xdb=10*log10(a0(i))
enddo
nsum=0
newdat=1 !Flag for new spectrum available
call zero(ss,nq) !Zero the accumulating array
if(jz.lt.300) jz=jz+1
endif
if(ndiskdat.eq.1) then
npts=jzc-kread
else
npts=iwrite-iread
if(npts.lt.0) npts=npts+nmax
endif
if(npts.ge.4096) go to 10
! Compute pixel values
iz=750
logmap=0
if(brightness.ne.b0 .or. contrast.ne.c0 .or. logmap.ne.logmap0 .or. &
nspeed.ne.nspeed0 .or. nlines.gt.1) then
iz=225000
gain=40*sqrt(nstep(nspeed)/5.0) * 5.0**(0.01*contrast)
gamma=1.3 + 0.01*contrast
offset=(brightness+64.0)/2
b0=brightness
c0=contrast
logmap0=logmap
nspeed0=nspeed
endif
! print*,brightness,contrast,logmap,gain,gamma,offset
do i=1,iz
n=0
if(a0(i).gt.0.0 .and. logmap.eq.1) n=gain*log10(0.001*a0(i)) + offset + 20
if(a0(i).gt.0.0 .and. logmap.eq.0) n=(0.01*a0(i))**gamma + offset
n=min(252,max(0,n))
a(i)=n
enddo
900 continue
return
end subroutine spec