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PROGRAM density
use netcdf
implicit none
c ---------------------------------------------------------------------
c Declaration of variables
c ---------------------------------------------------------------------
c Parameter and working arrays
real radius
character*80 runit
integer nx,ny
integer nlonlat
real dlonlat
real xmin,ymin,dx,dy
real clon,clat
integer ntime,nfield,ntra
character*80 inpfile
character*80 outfile
character*80 mode
real param
integer opts,npts
integer step
character*80 gridtype
character*80 field
integer crefile,crevar
real,allocatable, dimension (:,:) :: cnt,res,fld,area
real,allocatable, dimension (:) :: traj
real,allocatable, dimension (:) :: olon,olat,otim,ofld
real,allocatable, dimension (:) :: nlon,nlat,ntim,nfld
c Output format
character*80 outformat
c Physical and mathematical constants
real pi180
parameter (pi180=3.14159/180.)
real deltay
parameter (deltay=111.)
real eps
parameter (eps=0.001)
c Input trajectories (see iotra.f)
integer inpmode
real,allocatable, dimension (:,:,:) :: trainp
integer reftime(6)
character*80 varsinp(100)
integer,allocatable, dimension (:) :: sel_flag
character*80 sel_file
character*80 sel_format
c Auxiliary variables
character*80 cdfname,varname
integer i,j,k
integer stat
integer,allocatable, dimension (:,:) :: connect0
integer connectval0
integer,allocatable, dimension (:,:) :: connect1
integer connectval1
integer,allocatable, dimension (:,:) :: connect2
integer connectval2
real slat
integer ipre
real addvalue
real xmax,ymax
real ,allocatable, dimension (:) :: odist,ndist
real dt
integer fid
integer dynamic_grid
real ycen,xcen
integer indx,indy
character*80 unit
real pollon,pollat
real rlon0,rlat0,rlon,rlat
real lon,lat
real crot
integer count
character*80 longname, varunit
real time
integer ind
integer ifield
real hhmm,frac
integer ierr,ncID
c External functions
real lmstolm,lmtolms
real phstoph,phtophs
external lmstolm,lmtolms,phstoph,phtophs
real sdis
external sdis
c ---------------------------------------------------------------------
c Preparations
c ---------------------------------------------------------------------
c Write start message
print*,'========================================================='
print*,' *** START OF PROGRAM DENSITY ***'
print*
c Read input parameters
open(10,file='density.param')
read(10,*) inpfile
read(10,*) outfile
read(10,*) field
read(10,*) ntime,nfield,ntra
read(10,*) gridtype
if ( gridtype.eq.'latlon' ) then
read(10,*) nx,ny,xmin,ymin,dx,dy
elseif ( gridtype.eq.'rotated') then
read(10,*) clon,clat,nlonlat,dlonlat
else
print*,' ERROR: unsupported grid type ',trim(gridtype)
stop
endif
read(10,*) radius,runit
read(10,*) mode
read(10,*) param
read(10,*) step
read(10,*) sel_file
read(10,*) sel_format
read(10,*) crefile
read(10,*) crevar
close(10)
c Get the grid parameters if <crefile=0>
if ( crefile.eq.0 ) then
ierr = nf90_open (trim(outfile), NF90_NOWRITE , ncID)
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'grid' ,gridtype )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'clon' ,clon )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'clat' ,clat )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'nlonlat',nlonlat )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'dlonlat',dlonlat )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'nx' ,nx )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'ny' ,ny )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'dx' ,dx )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'dy' ,dy )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'xmin' ,xmin )
ierr = nf90_get_att(ncID, NF90_GLOBAL, 'ymin' ,ymin )
ierr = nf90_close(ncID)
print*,'**** GRID PARAMETERS IMPORTED ',
> 'FROM NETCDF FILE!!!! ****'
print*
endif
c Check for consistency
if ( (step.ne.0).and.(mode.ne.'keep') ) then
print*," ERROR: interpolation is only possible for all",
> ' time steps... Stop'
stop
endif
c Set the number of times (just code aesthetics)
opts=ntime
c Set grid parameters for rotated grid
if ( gridtype.eq.'rotated' ) then
nx = nlonlat
ny = nlonlat
dx = dlonlat
dy = dlonlat
xmin = - real(nlonlat-1)/2. * dx
xmax = + real(nlonlat-1)/2. * dx
ymin = - real(nlonlat-1)/2. * dy
ymax = + real(nlonlat-1)/2. * dy
endif
c Set the flag for dynamic grid adjustment
if ( (nx.eq.0).or.(ny.eq.0) ) then
dynamic_grid = 1
else
dynamic_grid = 0
endif
c Print status information
print*,'---- INPUT PARAMETERS -----------------------------------'
print*
print*,'Input : ',trim(inpfile)
print*,'Output : ',trim(outfile)
print*,'Field : ',trim(field)
print*,'Trajectory : ',ntime,nfield,ntra
print*,'Grid type : ',trim(gridtype)
if ( dynamic_grid.eq.1 ) then
print*,'Grid : dynamic (see below)'
elseif ( gridtype.eq.'latlon' ) then
print*,'Grid nlon,nlat : ',nx,ny
print*,' lonmin,latmin : ',xmin,ymin
print*,' dlon,dlat : ',dx,dy
elseif ( gridtype.eq.'rotated' ) then
print*,'Grid clon,clat : ',clon,clat
print*,' nlonlat : ',nlonlat
print*,' dlonlat : ',dlonlat
endif
print*,'Filter radius : ',radius,' ',trim(runit)
print*,'Mode : ',trim(mode)
if ( ( mode.eq.'time' ).or.
> ( mode.eq.'space' ).or.
> (mode.eq.'grid' ) )
>then
print*,'Parameter : ',param
endif
if ( step.eq.0 ) then
print*,'Time step : all'
elseif (step.gt.0) then
print*,'Time step : ',step
endif
print*,'Selection file : ',trim(sel_file)
print*,'Selection format : ',trim(sel_file)
print*,'Flag <crefile> : ',crefile
print*,'Flag <crevar> : ',crevar
c Check whether mode is valid
if ((mode.ne.'keep' ).and.
> (mode.ne.'time' ).and.
> (mode.ne.'space' ).and.
> (mode.ne.'grid' ))
>then
print*,' ERROR: Invalid mode ',trim(mode)
stop
endif
c Allocate memory for old and new (reparameterised) trajectory
allocate(olon(ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array olon ***'
allocate(olat(ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array olat ***'
allocate(otim(ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array otim ***'
allocate(nlon(1000*ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array nlon ***'
allocate(nlat(1000*ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array nlat ***'
allocate(ntim(1000*ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array ntim ***'
allocate(odist(ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array odist ***'
allocate(ndist(1000*ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array ndist ***'
allocate(ofld(ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array ofld ***'
allocate(nfld(1000*ntime),stat=stat)
if (stat.ne.0) print*,'*** error allocating array nfld ***'
c Allocate memory for complete trajectory set
allocate(trainp(ntra,ntime,nfield),stat=stat)
if (stat.ne.0) print*,'*** error allocating array trainp ***'
allocate(sel_flag(ntra),stat=stat)
if (stat.ne.0) print*,'*** error allocating array sel_flag ***'
c Allocate memory for auxiliary fields
allocate(traj(nfield),stat=stat)
if (stat.ne.0) print*,'*** error allocating array traj ***'
c Set the format of the input file
call mode_tra(inpmode,inpfile)
if (inpmode.eq.-1) inpmode=1
c Read the input trajectory file
call ropen_tra(fid,inpfile,ntra,ntime,nfield,
> reftime,varsinp,inpmode)
call read_tra (fid,trainp,ntra,ntime,nfield,inpmode)
call close_tra(fid,inpmode)
c Check that first four columns correspond to time,lon,lat,p
if ( (varsinp(1).ne.'time' ).or.
> (varsinp(2).ne.'xpos' ).and.(varsinp(2).ne.'lon' ).or.
> (varsinp(3).ne.'ypos' ).and.(varsinp(3).ne.'lat' ).or.
> (varsinp(4).ne.'ppos' ).and.(varsinp(4).ne.'p' ) )
>then
print*,' ERROR: problem with input trajectories ...'
stop
endif
varsinp(1) = 'TIME'
varsinp(2) = 'lon'
varsinp(3) = 'lat'
varsinp(4) = 'p'
c Get the index of the field (if needed)
if ( field.ne.'nil' ) then
ifield = 0
do i=1,nfield
if ( varsinp(i).eq.field ) ifield = i
enddo
if ( ifield.eq.0 ) then
print*,' ERROR: field ',trim(field),' not found... Stop'
stop
endif
endif
c Write some status information of the input trajectories
print*
print*,'---- INPUT TRAJECTORIES ---------------------------------'
print*
print*,' Reference time (year) : ',reftime(1)
print*,' (month) : ',reftime(2)
print*,' (day) : ',reftime(3)
print*,' (hour) : ',reftime(4)
print*,' (min) : ',reftime(5)
print*,' Time range (min) : ',reftime(6)
do i=1,nfield
if ( i.ne.ifield ) then
print*,' Var :',i,trim(varsinp(i))
else
print*,' Var :',i,trim(varsinp(i)),
> ' [ gridding ]'
endif
enddo
print*,' List of selected times'
do i=1,ntime
if ( (step.eq.0).or.(step.eq.i) ) then
print*,' ',i,' -> ',trainp(1,i,1)
endif
enddo
print*
c Select flag: all trajectories are selected
if ( sel_file.eq.'nil' ) then
do i=1,ntra
sel_flag(i) = 1
enddo
c Select flag: index file
elseif ( sel_format.eq.'index' ) then
do i=1,ntra
sel_flag(i) = 0
enddo
open(10,file=sel_file)
142 read(10,*,end=141) ind
sel_flag(ind) = 1
goto 142
141 continue
close(10)
c Select flag: boolean file
elseif ( sel_format.eq.'boolean' ) then
open(10,file=sel_file)
do i=1,ntra
read(10,*) ind
if ( ind.eq.1 ) sel_flag(i) = ind
enddo
close(10)
endif
c Write status information
if ( sel_file.eq.'nil' ) then
print*,' Selected trajectories : all ',ntra
else
count = 0
do i=1,ntra
if ( sel_flag(i).eq.1 ) count = count + 1
enddo
print*,' #selected trajectories : ',count,
> ' [ ',real(count)/real(ntra) * 100.,' % ] '
endif
print*
c ---------------------------------------------------------------------
c Coordinate transformations and grid adjustment
c ---------------------------------------------------------------------
c Transform from lat/lon to rotated lat/lon, if requested
if ( gridtype.eq.'rotated') then
crot = 0.
pollon=clon-180.
if (pollon.lt.-180.) pollon=pollon+360.
pollat=90.-clat
do i=1,ntra
do j=1,ntime
if ( sel_flag(i).eq.1 ) then
c Get lat/lon coordinates for trajectory point
lon = trainp(i,j,2)
lat = trainp(i,j,3)
c First Rotation
pollon=clon-180.
if (pollon.lt.-180.) pollon=pollon+360.
pollat=90.-clat
rlon0=lmtolms(lat,lon,pollat,pollon)
rlat0=phtophs(lat,lon,pollat,pollon)
c Second rotation
pollon=-180.
pollat=90.+crot
rlon=90.+lmtolms(rlat0,rlon0-90.,pollat,pollon)
rlat=phtophs(rlat0,rlon0-90.,pollat,pollon)
c Get rotated latitude and longitude
100 if (rlon.lt.xmin) then
rlon=rlon+360.
goto 100
endif
102 if (rlon.gt.(xmin+real(nx-1)*dx)) then
rlon=rlon-360.
goto 102
endif
c Set the new trajectory coordinates
trainp(i,j,2) = rlon
trainp(i,j,3) = rlat
endif
enddo
enddo
endif
c Dynamic grid adjustment
if ( dynamic_grid.eq.1 ) then
c Get the grid parameters
xmin = 180.
ymin = 90.
xmax = -180.
ymax = -90.
do i=1,ntra
if ( sel_flag(i).eq.1 ) then
if ( step.eq.0 ) then
do j=1,ntime
if ( trainp(i,j,2).lt.xmin) xmin = trainp(i,j,2)
if ( trainp(i,j,2).gt.xmax) xmax = trainp(i,j,2)
if ( trainp(i,j,3).lt.ymin) ymin = trainp(i,j,3)
if ( trainp(i,j,3).gt.ymax) ymax = trainp(i,j,3)
enddo
else
if ( trainp(i,step,2).lt.xmin) xmin = trainp(i,step,2)
if ( trainp(i,step,2).gt.xmax) xmax = trainp(i,step,2)
if ( trainp(i,step,3).lt.ymin) ymin = trainp(i,step,3)
if ( trainp(i,step,3).gt.ymax) ymax = trainp(i,step,3)
endif
endif
enddo
c Get first guess for "optimal" grid
nx = 400
ny = 400
dx = (xmax - xmin)/real(nx-1)
dy = (ymax - ymin)/real(ny-1)
c Make the grid spacing equal in zonal and meridional direction
if ( dx.gt.dy ) then
dy = dx
ny = (ymax - ymin)/dy + 1
if (ny.lt.nx/2) ny = nx / 2
if ( real(ny)*dy .ge. 180. ) ny = 180./dy + 1
ycen = 0.5* (ymin+ymax)
ymin = ycen - 0.5 * real(ny/2) * dy
if (ymin.le.-90.) ymin = -90.
else
dx = dy
nx = (xmax - xmin)/dx + 1
if (nx.lt.ny/2) nx = ny / 2
if ( real(nx)*dx .ge. 360. ) nx = 360./dx + 1
xcen = 0.5* (xmin+xmax)
xmin = xcen - 0.5 * real(nx/2) * dx
if (xmin.le.-180.) xmin = -180.
endif
c Write information
print*
print*,'---- DYNAMIC GRID ADJUSTMENT',
> ' ----------------------------'
print*
print*,'Grid nlon,nlat : ',nx,ny
print*,' lonmin,latmin : ',xmin,ymin
print*,' dlon,dlat : ',dx,dy
print*
c Write grid information for rotated grid (if not already done
elseif ( gridtype.eq.'rotated') then
print*
print*,'---- GRID PARAMETERS -------',
> ' ----------------------------'
print*
print*,'Grid nlon,nlat : ',nx,ny
print*,' lonmin,latmin : ',xmin,ymin
print*,' dlon,dlat : ',dx,dy
print*
endif
c Set the grid boundaries
xmax=xmin+real(nx-1)*dx
ymax=ymin+real(ny-1)*dy
c Allocate memory for output array and auxiliary gridding array
allocate(cnt(nx,ny),stat=stat)
if (stat.ne.0) print*,'*** error allocating array cnt ***'
allocate(res(nx,ny),stat=stat)
if (stat.ne.0) print*,'*** error allocating array res ***'
allocate(fld(nx,ny),stat=stat)
if (stat.ne.0) print*,'*** error allocating array fld ***'
allocate(area(nx,ny),stat=stat)
if (stat.ne.0) print*,'*** error allocating array area ***'
allocate(connect0(nx,ny),stat=stat)
if (stat.ne.0) print*,'*** error allocating array connect0 ***'
allocate(connect1(nx,ny),stat=stat)
if (stat.ne.0) print*,'*** error allocating array connect1 ***'
allocate(connect2(nx,ny),stat=stat)
if (stat.ne.0) print*,'*** error allocating array connect2 ***'
c Init the output array
do i=1,nx
do j=1,ny
connect0(i,j) = 0
connect1(i,j) = 0
connect2(i,j) = 0
cnt(i,j) = 0.
res(i,j) = 0.
fld(i,j) = 0.
enddo
enddo
c ---------------------------------------------------------------------
c Gridding
c ---------------------------------------------------------------------
c Write some status information
print*,'---- GRIDDING -------------------------------------------'
print*
c Loop over all entries of sampling table
connectval0 = 0
connectval1 = 0
connectval2 = 0
count = 0
do i=1,ntra
if (mod(i,100).eq.0) print*,i,' of ',ntra
c Skip all trajectories which are not selected
if ( sel_flag(i).eq.0 ) goto 300
c ------- Read a complete trajectory ---------------------------
do j=1,ntime
otim(j) = trainp(i,j,1)
olon(j) = trainp(i,j,2)
olat(j) = trainp(i,j,3)
if ( field.ne.'nil' ) then
ofld(j) =trainp(i,j,ifield)
endif
enddo
c -------- Convert hh.m time into fractional time --------------
do j=1,ntime
hhmm = otim(j)
call hhmm2frac (hhmm,frac)
otim(j) = frac
enddo
c -------- Interpolation ---------------------------------------
c Keep the trajectory points as they are
if ( ( mode.eq.'keep').and.(step.eq.0) ) then
npts=opts
do j=1,opts
ntim(j)=otim(j)
nlon(j)=olon(j)
nlat(j)=olat(j)
if ( field.ne.'nil' ) then
nfld(j)=ofld(j)
endif
enddo
c Select a single time step
elseif ( ( mode.eq.'keep').and.(step.gt.0) ) then
npts = 1
ntim(1) = otim(step)
nlon(1) = olon(step)
nlat(1) = olat(step)
if ( field.ne.'nil' ) then
nfld(1) = ofld(step)
endif
c Perform a reparameterisation in time
else if ( (mode.eq.'time').and.(step.eq.0) ) then
c Get the new number of trajectory points
npts=nint(abs(otim(opts)-otim(1))/param)+1
c Handle date line problem
do j=2,opts
if ( (olon(j-1)-olon(j)).gt.180. ) then
olon(j) = olon(j) + 360.
else if ( (olon(j-1)-olon(j)).lt.-180. ) then
olon(j) = olon(j) - 360.
endif
enddo
c Cubic spline fitting
call curvefit(otim,olon,opts,ntim,nlon,npts)
call curvefit(otim,olat,opts,ntim,nlat,npts)
if ( field.ne.'nil' ) then
call curvefit(otim,ofld,opts,ntim,nfld,npts)
endif
c Reverse date line handling
do j=1,npts
if ( nlon(j).gt.xmax ) then
nlon(j) = nlon(j) -360.
else if ( nlon(j).lt.xmin ) then
nlon(j) = nlon(j) +360.
endif
enddo
c Perform a reparameterisation with equally spaced gridpoint
elseif ( (mode.eq.'space').and.(step.eq.0) ) then
c Calculate the distance and spacing
odist(1) = 0.
unit = 'km'
do j=2,ntime
odist(j)=odist(j-1) +
> sdis(olon(j-1),olat(j-1),olon(j),olat(j),unit)
enddo
c Determine the new number of trajectory points
npts=nint(odist(ntime)/param)+1
if (npts.eq.0) then
npts=1.
endif
c Handle date line problem
do j=2,opts
if ( (olon(j-1)-olon(j)).gt.180. ) then
olon(j) = olon(j) + 360.
else if ( (olon(j-1)-olon(j)).lt.-180. ) then
olon(j) = olon(j) - 360.
endif
enddo
c Cubic spline fitting
call curvefit(odist,olon,opts,ndist,nlon,npts)
call curvefit(odist,olat,opts,ndist,nlat,npts)
call curvefit(odist,otim,opts,ndist,ntim,npts)
if ( field.ne.'nil' ) then
call curvefit(odist,ofld,opts,ndist,nfld,npts)
endif
c Reverse date line handling
do j=1,npts
if ( nlon(j).gt.xmax ) then
nlon(j) = nlon(j) -360.
else if ( nlon(j).lt.xmin ) then
nlon(j) = nlon(j) +360.
endif
enddo
c Perform a reparameterisation with equally spaced gridpoint
elseif ( (mode.eq.'grid').and.(step.eq.0) ) then
c Calculate the distance and spacing
odist(1) = 0.
unit = 'deg'
do j=2,ntime
odist(j)=odist(j-1) +
> sdis(olon(j-1),olat(j-1),olon(j),olat(j),unit)
enddo
c Determine the new number of trajectory points
npts=nint(odist(ntime)/param)+1
if (npts.eq.0) then
npts=1.
endif
c Handle date line problem
do j=2,opts
if ( (olon(j-1)-olon(j)).gt.180. ) then
olon(j) = olon(j) + 360.
else if ( (olon(j-1)-olon(j)).lt.-180. ) then
olon(j) = olon(j) - 360.
endif
enddo
c Cubic spline fitting
call curvefit(odist,olon,opts,ndist,nlon,npts)
call curvefit(odist,olat,opts,ndist,nlat,npts)
call curvefit(odist,otim,opts,ndist,ntim,npts)
if ( field.ne.'nil' ) then
call curvefit(odist,ofld,opts,ndist,nfld,npts)
endif
c Reverse date line handling
do j=1,npts
if ( nlon(j).gt.xmax ) then
nlon(j) = nlon(j) -360.
else if ( nlon(j).lt.xmin ) then
nlon(j) = nlon(j) +360.
endif
enddo
endif
c -------- Do the gridding -------------------------------------
c Gridding of trajectory
do j=1,npts
c Check whether point is in data domain
if ( (nlon(j).gt.xmin).and.(nlon(j).lt.xmax).and.
> (nlat(j).gt.ymin).and.(nlat(j).lt.ymax))
> then
c Increase counter for gridded points
count = count + 1
c ----------------- Gridding: simple count -----------------
connectval0 = connectval0+1
addvalue = 1.
call gridding1
> (nlat(j),nlon(j),addvalue,
> radius,runit,connect0,connectval0,
> cnt,nx,ny,xmin,ymin,dx,dy)
c ----------------- Gridding: residence time ---------------
connectval1 = connectval1+1
if ( ntime.eq.1 ) then
addvalue = 0.
elseif ( j.eq.1 ) then
addvalue=abs(ntim(2)-ntim(1))
else
addvalue=abs(ntim(j)-ntim(j-1))
endif
call gridding1
> (nlat(j),nlon(j),addvalue,
> radius,runit,connect1,connectval1,
> res,nx,ny,xmin,ymin,dx,dy)
c --------------- Gridding: field -------------------------
if ( field.ne.'nil' ) then
connectval2 = connectval2+1
addvalue = nfld(j)
call gridding1
> (nlat(j),nlon(j),addvalue,
> radius,runit,connect2,connectval2,
> fld,nx,ny,xmin,ymin,dx,dy)
endif
endif
enddo
c Exit point for loop over all trajectories
300 continue
enddo
c Write status information
print*
print*,' # gridded points : ',count
c ---------------------------------------------------------------------
c Unit conversions and output to netCDF file
c ---------------------------------------------------------------------
c Write some status information
print*
print*,'---- WRITE OUTPUT ---------------------------------------'
print*
c Area (in km^2)
do i=1,nx
do j=1,ny
slat=ymin+real(j-1)*dy
if (abs(abs(slat)-90.).gt.eps) then
area(i,j) = dy*dx*cos(pi180*slat)*deltay**2
else
area(i,j) = 0.
endif
enddo
enddo
c Normalise gridded field
if ( field.ne.'nil' ) then
do i=1,nx
do j=1,ny
if ( cnt(i,j).gt.0. ) then
fld(i,j) = fld(i,j) / cnt(i,j)
endif
enddo
enddo
endif
c Set the time for the output netCDF files - if a composite is
c calculatd, then the time is set to
if ( step.eq.0 ) then
time = -999.
print*,' ... COMPOSITE OVER ALL TRAJECTORY TIMES (-999)'
print*
else
time = trainp(1,step,1)
endif
c Write output to CF netCDF
cdfname = outfile
varname = 'COUNT'
longname = 'trajectory counts'
varunit = 'counts per grid point'
call writecdf2D_cf (cdfname,varname,longname,varunit,gridtype,
> clon,clat,nlonlat,dlonlat,cnt,time,dx,dy,xmin,ymin,nx,
> ny,crefile,crefile,1)
write(*,'(a8,a10,a5,a10,a10,f7.2,a2)')
> ' ... ',trim(varname),' -> ',trim(cdfname),
> ' [ time = ',time,' ]'
varname = 'RESIDENCE'
longname = 'residence time'
varunit = 'hours per grid point'
print*,'crefile = ',crefile
call writecdf2D_cf (cdfname,varname,longname,varunit,gridtype,
> clon,clat,nlonlat,dlonlat,res,time,dx,dy,xmin,ymin,nx,
> ny,0,crefile,1)
write(*,'(a8,a10,a5,a10,a10,f7.2,a2)')
> ' ... ',trim(varname),' -> ',trim(cdfname),
> ' [ time = ',time,' ]'
varname = 'AREA'
longname = 'area corresponding to grid points'
varunit = 'square kilometers'
call writecdf2D_cf (cdfname,varname,longname,varunit,gridtype,
> clon,clat,nlonlat,dlonlat,area,time,dx,dy,xmin,ymin,nx,
> ny,0,crefile,1)
write(*,'(a8,a10,a5,a10,a10,f7.2,a2)')
> ' ... ',trim(varname),' -> ',trim(cdfname),
> ' [ time = ',time,' ]'
if ( field.ne.'nil' ) then
varname = field
longname = field
varunit = 'as on trajectory file'
call writecdf2D_cf (cdfname,varname,longname,varunit,gridtype,
> clon,clat,nlonlat,dlonlat,fld,time,dx,dy,xmin,ymin,nx,
> ny,0,crevar,1)
write(*,'(a8,a10,a5,a10,a10,f7.2,a2)')
> ' ... ',trim(varname),' -> ',trim(cdfname),
> ' [ time = ',time,' ]'
endif
c Write status information
print*
print*,' *** END OF PROGRAM DENSITY **'
print*,'========================================================='
end
c ********************************************************************
c * GRIDDING SUBROUTINES *
c ********************************************************************
c ---------------------------------------------------------------------
c Gridding of one single data point (smoothing in km, deg, gridp)
c ---------------------------------------------------------------------
subroutine gridding1 (lat,lon,addval,radius,unit,
> connect,connectval,
> out,nx,ny,xmin,ymin,dx,dy)
implicit none
c Declaration of subroutine parameters
real lat,lon
integer nx,ny
real xmin,ymin,dx,dy
real out(nx,ny)
real radius
character*80 unit
integer connectval
integer connect(nx,ny)
real addval
c Auxiliary variables
integer i,j,k
integer mu,md,nr,nl,n,m
integer stackx(nx*ny),stacky(nx*ny)
integer tab_x(nx*ny),tab_y(nx*ny)
real tab_r(nx*ny)
integer sp
real lat2,lon2
real dist,sum
real xmax
integer periodic
integer test
c Numerical epsilon
real eps
parameter (eps=0.01)
c Externals
real sdis,weight
external sdis,weight
c Check whether lat/lon point is valid
xmax=xmin+real(nx-1)*dx
if (lon.lt.xmin-eps) lon=lon+360.
if (lon.gt.xmax+eps) lon=lon-360.
if (abs(lat-90).lt.eps) lat=90.
if (abs(lat+90).lt.eps) lat=-90.
if ((abs(lat).gt.(90.+eps)).or.
> (lon.lt.xmin-eps).or.(lon.gt.xmax+eps)) then
print*,'Invalid lat/lon point ',lat,lon
return
endif
c Set flag for periodic domain
if (abs(xmax-xmin-360.).lt.eps) then
periodic=1
else if (abs(xmax-xmin-360+dx).lt.eps) then
periodic=2
else
periodic=0
endif
c Get indices of one coarse grid point within search radius
i=nint((lon-xmin)/dx)+1
if ((i.eq.nx).and.(periodic.eq.1)) i=1
j=nint((lat-ymin)/dy)+1
lat2=ymin+real(j-1)*dy
lon2=xmin+real(i-1)*dx
dist=sdis(lon,lat,lon2,lat2,unit)
if (dist.gt.radius) then
print*,'1: Search radius is too small...'
stop
endif
c Get connected points
k=0
stackx(1)=i
stacky(1)=j
sp=1
do while (sp.ne.0)
c Get an element from stack
n=stackx(sp)
m=stacky(sp)
sp=sp-1
c Get distance from reference point
lat2=ymin+real(m-1)*dy
lon2=xmin+real(n-1)*dx
dist=sdis(lon,lat,lon2,lat2,unit)
c Check whether distance is smaller than search radius: connected
if (dist.lt.radius) then
c Make entry in filter mask
k=k+1
tab_x(k)=n
tab_y(k)=m
tab_r(k)=weight(dist,radius)
c Mark this point as visited
connect(n,m)=connectval
c Get coordinates of neighbouring points
nr=n+1
if ((nr.gt.nx) .and.(periodic.eq.0)) nr=nx
if ((nr.gt.nx-1).and.(periodic.eq.1)) nr=1
if ((nr.gt.nx) .and.(periodic.eq.2)) nr=1
nl=n-1
if ((nl.lt.1).and.(periodic.eq.0)) nl=1
if ((nl.lt.1).and.(periodic.eq.1)) nl=nx-1
if ((nl.lt.1).and.(periodic.eq.2)) nl=nx
mu=m+1
if (mu.gt.ny) mu=ny
md=m-1
if (md.lt.1) md=1
c Update stack
if (connect(nr,m).ne.connectval) then
connect(nr,m)=connectval
sp=sp+1
stackx(sp)=nr
stacky(sp)=m
endif
if (connect(nl,m).ne.connectval) then
connect(nl,m)=connectval
sp=sp+1
stackx(sp)=nl
stacky(sp)=m
endif
if (connect(n,mu).ne.connectval) then
connect(n,mu)=connectval
sp=sp+1
stackx(sp)=n
stacky(sp)=mu
endif
if (connect(n,md).ne.connectval) then
connect(n,md)=connectval
sp=sp+1
stackx(sp)=n
stacky(sp)=md
endif
endif
end do
if (k.ge.1) then
sum=0.
do i=1,k
sum=sum+tab_r(i)
enddo
do i=1,k
out(tab_x(i),tab_y(i))=out(tab_x(i),tab_y(i))+
> addval*tab_r(i)/sum
if ((tab_x(i).eq.1).and.(periodic.eq.1)) then
out(nx,tab_y(i))=out(nx,tab_y(i))+
> addval*tab_r(i)/sum
endif
enddo
else
print*,'2: Search radius is too small...'
stop
endif
end
c ----------------------------------------------------------------------
c Get spherical distance between lat/lon points
c ----------------------------------------------------------------------
real function sdis(xp,yp,xq,yq,unit)
c Calculates spherical distance (in km) between two points given
c by their spherical coordinates (xp,yp) and (xq,yq), respectively.
real re
parameter (re=6370.)
real xp,yp,xq,yq,arg
character*80 unit
real dlon
if ( unit.eq.'km' ) then
arg=sind(yp)*sind(yq)+cosd(yp)*cosd(yq)*cosd(xp-xq)
if (arg.lt.-1.) arg=-1.
if (arg.gt.1.) arg=1.
sdis=re*acos(arg)
elseif ( unit.eq.'deg' ) then
dlon = xp-xq
if ( dlon.gt. 180. ) dlon = dlon - 360.
if ( dlon.lt.-180. ) dlon = dlon + 360.
sdis = sqrt( dlon**2 + (yp-yq)**2 )
endif
c Quick and dirty trick to avoid zero distances
if (sdis.eq.0.) sdis=0.1
end
c ----------------------------------------------------------------------
c Weight function for the filter mask
c ----------------------------------------------------------------------
real function weight (r,radius)
c Attribute to each distanc r its corresponding weight in the filter mask
implicit none
c Declaration of subroutine parameters
real r
real radius
c Simple 0/1 mask
if (r.lt.radius) then
weight=exp(-r/radius)
else
weight=0.
endif
end
c ********************************************************************
c * REPARAMETERIZATION SUBROUTINES *
c ********************************************************************
c -------------------------------------------------------------
c Interpolation of the trajectory with a natural cubic spline
c -------------------------------------------------------------
SUBROUTINE curvefit (time,lon,n,
> sptime,splon,spn)
c Given the curve <time,lon> with <n> data points, fit a
c cubic spline to this curve. The new curve is returned in
c <sptime,splon,spn> with <spn> data points. The parameter
c <spn> specifies on entry the number of spline interpolated points
c along the curve.
implicit none
c Declaration of subroutine parameters
integer n
real time(n),lon(n)
integer spn
real sptime(spn),splon(spn)
c Auxiliary variables
real y2ax(n)
real dt
real s
integer i
real order
c Determine whether the input array is ascending or descending
if (time(1).gt.time(n)) then
order=-1.
else
order= 1.
endif
c Bring the time array into ascending order
do i=1,n
time(i)=order*time(i)
enddo
c Prepare the (natural) cubic spline interpolation
call spline (time,lon,n,1.e30,1.e30,y2ax)
dt=(time(n)-time(1))/real(spn-1)
do i=1,spn
sptime(i)=time(1)+real(i-1)*dt
enddo
c Do the spline interpolation
do i=1,spn
call splint(time,lon,y2ax,n,sptime(i),s)
splon(i)=s
enddo
c Change the time arrays back
do i=1,spn
sptime(i)=order*sptime(i)
enddo
do i=1,n
time(i)=order*time(i)
enddo
return
end
c -------------------------------------------------------------
c Basic routines for spline interpolation (Numerical Recipes)
c -------------------------------------------------------------
SUBROUTINE spline(x,y,n,yp1,ypn,y2)
INTEGER n,NMAX
REAL yp1,ypn,x(n),y(n),y2(n)
PARAMETER (NMAX=500)
INTEGER i,k
REAL p,qn,sig,un,u(NMAX)
if (yp1.gt..99e30) then
y2(1)=0.
u(1)=0.
else
y2(1)=-0.5
u(1)=(3./(x(2)-x(1)))*((y(2)-y(1))/(x(2)-x(1))-yp1)
endif
do 11 i=2,n-1
sig=(x(i)-x(i-1))/(x(i+1)-x(i-1))
p=sig*y2(i-1)+2.
y2(i)=(sig-1.)/p
u(i)=(6.*((y(i+1)-y(i))/(x(i+
*1)-x(i))-(y(i)-y(i-1))/(x(i)-x(i-1)))/(x(i+1)-x(i-1))-sig*
*u(i-1))/p
11 continue
if (ypn.gt..99e30) then
qn=0.
un=0.
else
qn=0.5
un=(3./(x(n)-x(n-1)))*(ypn-(y(n)-y(n-1))/(x(n)-x(n-1)))
endif
y2(n)=(un-qn*u(n-1))/(qn*y2(n-1)+1.)
do 12 k=n-1,1,-1
y2(k)=y2(k)*y2(k+1)+u(k)
12 continue
return
END
SUBROUTINE splint(xa,ya,y2a,n,x,y)
INTEGER n
REAL x,y,xa(n),y2a(n),ya(n)
INTEGER k,khi,klo
REAL a,b,h
klo=1
khi=n
1 if (khi-klo.gt.1) then
k=(khi+klo)/2
if(xa(k).gt.x)then
khi=k
else
klo=k
endif
goto 1
endif
h=xa(khi)-xa(klo)
if (h.eq.0.) then
print*,'bad xa input in splint'
stop
endif
a=(xa(khi)-x)/h
b=(x-xa(klo))/h
y=a*ya(klo)+b*ya(khi)+((a**3-a)*y2a(klo)+(b**3-b)*y2a(khi))*(h**
*2)/6.
return
END
c ********************************************************************
c * INPUT / OUTPUT SUBROUTINES *
c ********************************************************************
c --------------------------------------------------------------------
c Subroutines to write the CF netcdf output file
c --------------------------------------------------------------------
subroutine writecdf2D_cf
> (cdfname,varname,longname,unit,gridtype,clon,clat,
> nlonlat,dlonlat,arr,time,dx,dy,xmin,ymin,nx,ny,
> crefile,crevar,cretime)
c Create and write to the CF netcdf file <cdfname>. The variable
c with name <varname> and with time <time> is written. The data
c are in the two-dimensional array <arr>. The list <dx,dy,xmin,
c ymin,nx,ny> specifies the output grid. The flags <crefile> and
c <crevar> determine whether the file and/or the variable should
c be created; correspondingly for the unlimited dimension <time>
c with the flag <cretime>.
USE netcdf
IMPLICIT NONE
c Declaration of input parameters
character*80 cdfname
character*80 varname,longname,unit
integer nx,ny
real arr(nx,ny)
real dx,dy,xmin,ymin
real time
integer crefile,crevar,cretime
character*80 gridtype
real clon,clat
integer nlonlat
real dlonlat
c Local variables
integer ierr
integer ncID
integer LonDimId, varLonID
integer LatDimID, varLatID
integer TimeDimID, varTimeID
real longitude(nx)
real latitude (ny)
real timeindex
integer i
integer nvars,varids(100)
integer ndims,dimids(100)
real timelist(1000)
integer ntimes
integer ind
integer varID
c Quick an dirty solution for fieldname conflict
if ( varname.eq.'time' ) varname = 'TIME'
c Initially set error to indicate no errors.
ierr = 0
c ---- Create the netCDF - skip if <crefile=0> ----------------------
if ( crefile.ne.1 ) goto 100
c Create the file
ierr = nf90_create(trim(cdfname), NF90_CLOBBER, ncID)
c Define dimensions
ierr=nf90_def_dim(ncID,'longitude',nx , LonDimID )
ierr=nf90_def_dim(ncID,'latitude' ,ny , LatDimID )
ierr=nf90_def_dim(ncID,'time' ,nf90_unlimited, TimeDimID)
c Define coordinate Variables
ierr = nf90_def_var(ncID,'longitude',NF90_FLOAT,
> (/ LonDimID /),varLonID)
ierr = nf90_put_att(ncID, varLonID, "standard_name","longitude")
ierr = nf90_put_att(ncID, varLonID, "units" ,"degree_east")
ierr = nf90_def_var(ncID,'latitude',NF90_FLOAT,
> (/ LatDimID /),varLatID)
ierr = nf90_put_att(ncID, varLatID, "standard_name", "latitude")
ierr = nf90_put_att(ncID, varLatID, "units" ,"degree_north")
ierr = nf90_def_var(ncID,'time',NF90_FLOAT,
> (/ TimeDimID /), varTimeID)
ierr = nf90_put_att(ncID, varTimeID, "axis", "T")
ierr = nf90_put_att(ncID, varTimeID, "calendar", "standard")
ierr = nf90_put_att(ncID, varTimeID, "long_name", "time")
ierr = nf90_put_att(ncID, varTimeID, "units", "hours")
c Write global attributes
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'Conventions', 'CF-1.0')
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'title',
> 'Trajectory Densities')
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'source',
> 'Lagranto Trajectories')
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'institution',
> 'ETH Zurich, IACETH')
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'grid',trim(gridtype) )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'clon',clon )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'clat',clat )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'nlonlat',nlonlat )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'dlonlat',dlonlat )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'nx',nx )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'ny',ny )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'dx',dx )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'dy',dy )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'xmin',xmin )
ierr = nf90_put_att(ncID, NF90_GLOBAL, 'ymin',ymin )
c Write coordinate data
do i = 1,nx+1
longitude(i) = xmin + real(i-1) * dx
enddo
do i = 1,ny+1
latitude(i) = ymin + real(i-1) * dy
enddo
c Check whether the definition was successful
ierr = nf90_enddef(ncID)
if (ierr.gt.0) then
print*, 'An error occurred while attempting to ',
> 'finish definition mode.'
stop
endif
c Write coordinate data
ierr = nf90_put_var(ncID,varLonID ,longitude)
ierr = nf90_put_var(ncID,varLatID ,latitude )
c Close netCDF file
ierr = nf90_close(ncID)
100 continue
c ---- Define a new variable - skip if <crevar=0> -----------------------
if ( crevar.ne.1 ) goto 110
c Open the file for read(write access
ierr = nf90_open (trim(cdfname), NF90_WRITE , ncID)
c Get the IDs for dimensions
ierr = nf90_inq_dimid(ncID,'longitude', LonDimID )
ierr = nf90_inq_dimid(ncID,'latitude' , LatDimID )
ierr = nf90_inq_dimid(ncID,'time' , TimeDimID)
c Enter define mode
ierr = nf90_redef(ncID)
c Write definition and add attributes
ierr = nf90_def_var(ncID,varname,NF90_FLOAT,
> (/ LonDimID, LatDimID, TimeDimID /),varID)
ierr = nf90_put_att(ncID, varID, "long_name" , longname )
ierr = nf90_put_att(ncID, varID, "units" , unit )
ierr = nf90_put_att(ncID, varID, '_FillValue', -999.99 )
c Check whether definition was successful
ierr = nf90_enddef(ncID)
if (ierr.gt.0) then
print*, 'An error occurred while attempting to ',
> 'finish definition mode.'
stop
endif
print*,trim(varname),' defined on ',trim(cdfname)
c Close netCDF file
ierr = nf90_close(ncID)
110 continue
c ---- Create a new time (unlimited dimension) - skip if <cretime=0> ------
if ( cretime.ne.1 ) goto 120
c Open the file for read/write access
ierr = nf90_open (trim(cdfname), NF90_WRITE, ncID)
c Get the list of times on the netCDF file
ierr = nf90_inq_dimid(ncID,'time', TimeDimID)
if ( ierr.ne.0 ) then
print*,'Time dimension is not defined on ',trim(cdfname),
> ' .... Stop'
stop
endif
ierr = nf90_inquire_dimension(ncID, TimeDimID, len = ntimes)
ierr = nf90_inq_varid(ncID,'time', varTimeID)
if ( ierr.ne.0 ) then
print*,'Variable time is not defined on ',trim(cdfname),
> ' ... Stop'
stop
endif
ierr = nf90_get_var(ncID,varTimeID,timelist(1:ntimes))
c Decide whether a new time must be written
ind = 0
do i=1,ntimes
if ( time.eq.timelist(i) ) ind = i
enddo
c Extend the time list if required
if ( ind.eq.0 ) then
ntimes = ntimes + 1
timelist(ntimes) = time
ierr = nf90_put_var(ncID,varTimeID,timelist(1:ntimes))
endif
c Close netCDF file
ierr = nf90_close(ncID)
120 continue
c ---- Write data --------------------------------------------------
c Open the file for read/write access
ierr = nf90_open (trim(cdfname), NF90_WRITE , ncID)
c Get the varID
ierr = nf90_inq_varid(ncID,varname, varID )
if (ierr.ne.0) then
print*,'Variable ',trim(varname),' is not defined on ',
> trim(cdfname)
stop
endif
c Get the time index
ierr = nf90_inq_dimid(ncID,'time', TimeDimID)
if ( ierr.ne.0 ) then
print*,'Time dimension is not defined on ',trim(cdfname),
> ' .... Stop'
stop
endif
ierr = nf90_inquire_dimension(ncID, TimeDimID, len = ntimes)
ierr = nf90_inq_varid(ncID,'time', varTimeID)
if ( ierr.ne.0 ) then
print*,'Variable time is not defined on ',trim(cdfname),
> ' ... Stop'
stop
endif
ierr = nf90_get_var(ncID,varTimeID,timelist(1:ntimes))
ind = 0
do i=1,ntimes
if ( time.eq.timelist(i) ) ind = i
enddo
if (ind.eq.0) then
print*,'Time',time,' is not defined on the netCDF file',
> trim(cdfname),' ... Stop'
stop
endif
c Write data block
ierr = nf90_put_var(ncID,varID,arr,
> start = (/ 1, 1, ind /),
> count = (/ nx, ny, 1 /) )
c Check whether writing was successful
ierr = nf90_close(ncID)
if (ierr.ne.0) then
write(*,*) trim(nf90_strerror(ierr))
write(*,*) 'An error occurred while attempting to ',
> 'close the netcdf file.'
write(*,*) 'in clscdf_CF'
endif
end
c ********************************************************************************
c * Transformation routine: LMSTOLM and PHSTOPH from library gm2em *
c ********************************************************************************
REAL FUNCTION LMSTOLM (PHIS, LAMS, POLPHI, POLLAM)
C
C**** LMSTOLM - FC:BERECHNUNG DER WAHREN GEOGRAPHISCHEN LAENGE FUER
C**** EINEN PUNKT MIT DEN KOORDINATEN (PHIS, LAMS)
C**** IM ROTIERTEN SYSTEM. DER NORDPOL DES SYSTEMS HAT
C**** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** AUFRUF : LAM = LMSTOLM (PHIS, LAMS, POLPHI, POLLAM)
C** ENTRIES : KEINE
C** ZWECK : BERECHNUNG DER WAHREN GEOGRAPHISCHEN LAENGE FUER
C** EINEN PUNKT MIT DEN KOORDINATEN (PHIS, LAMS)
C** IM ROTIERTEN SYSTEM. DER NORDPOL DIESES SYSTEMS HAT
C** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** VERSIONS-
C** DATUM : 03.05.90
C**
C** EXTERNALS: KEINE
C** EINGABE-
C** PARAMETER: PHIS REAL GEOGR. BREITE DES PUNKTES IM ROT.SYS.
C** LAMS REAL GEOGR. LAENGE DES PUNKTES IM ROT.SYS.
C** POLPHI REAL WAHRE GEOGR. BREITE DES NORDPOLS
C** POLLAM REAL WAHRE GEOGR. LAENGE DES NORDPOLS
C** AUSGABE-
C** PARAMETER: WAHRE GEOGRAPHISCHE LAENGE ALS WERT DER FUNKTION
C** ALLE WINKEL IN GRAD (NORDEN>0, OSTEN>0)
C**
C** COMMON-
C** BLOECKE : KEINE
C**
C** FEHLERBE-
C** HANDLUNG : KEINE
C** VERFASSER: D.MAJEWSKI
REAL LAMS,PHIS,POLPHI,POLLAM
DATA ZRPI18 , ZPIR18 / 57.2957795 , 0.0174532925 /
ZSINPOL = SIN(ZPIR18*POLPHI)
ZCOSPOL = COS(ZPIR18*POLPHI)
ZLAMPOL = ZPIR18*POLLAM
ZPHIS = ZPIR18*PHIS
ZLAMS = LAMS
IF(ZLAMS.GT.180.0) ZLAMS = ZLAMS - 360.0
ZLAMS = ZPIR18*ZLAMS
ZARG1 = SIN(ZLAMPOL)*(- ZSINPOL*COS(ZLAMS)*COS(ZPHIS) +
1 ZCOSPOL* SIN(ZPHIS)) -
2 COS(ZLAMPOL)* SIN(ZLAMS)*COS(ZPHIS)
ZARG2 = COS(ZLAMPOL)*(- ZSINPOL*COS(ZLAMS)*COS(ZPHIS) +
1 ZCOSPOL* SIN(ZPHIS)) +
2 SIN(ZLAMPOL)* SIN(ZLAMS)*COS(ZPHIS)
IF (ABS(ZARG2).LT.1.E-30) THEN
IF (ABS(ZARG1).LT.1.E-30) THEN
LMSTOLM = 0.0
ELSEIF (ZARG1.GT.0.) THEN
LMSTOLAM = 90.0
ELSE
LMSTOLAM = -90.0
ENDIF
ELSE
LMSTOLM = ZRPI18*ATAN2(ZARG1,ZARG2)
ENDIF
RETURN
END
REAL FUNCTION PHSTOPH (PHIS, LAMS, POLPHI, POLLAM)
C
C**** PHSTOPH - FC:BERECHNUNG DER WAHREN GEOGRAPHISCHEN BREITE FUER
C**** EINEN PUNKT MIT DEN KOORDINATEN (PHIS, LAMS) IM
C**** ROTIERTEN SYSTEM. DER NORDPOL DIESES SYSTEMS HAT
C**** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** AUFRUF : PHI = PHSTOPH (PHIS, LAMS, POLPHI, POLLAM)
C** ENTRIES : KEINE
C** ZWECK : BERECHNUNG DER WAHREN GEOGRAPHISCHEN BREITE FUER
C** EINEN PUNKT MIT DEN KOORDINATEN (PHIS, LAMS) IM
C** ROTIERTEN SYSTEM. DER NORDPOL DIESES SYSTEMS HAT
C** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** VERSIONS-
C** DATUM : 03.05.90
C**
C** EXTERNALS: KEINE
C** EINGABE-
C** PARAMETER: PHIS REAL GEOGR. BREITE DES PUNKTES IM ROT.SYS.
C** LAMS REAL GEOGR. LAENGE DES PUNKTES IM ROT.SYS.
C** POLPHI REAL WAHRE GEOGR. BREITE DES NORDPOLS
C** POLLAM REAL WAHRE GEOGR. LAENGE DES NORDPOLS
C** AUSGABE-
C** PARAMETER: WAHRE GEOGRAPHISCHE BREITE ALS WERT DER FUNKTION
C** ALLE WINKEL IN GRAD (NORDEN>0, OSTEN>0)
C**
C** COMMON-
C** BLOECKE : KEINE
C**
C** FEHLERBE-
C** HANDLUNG : KEINE
C** VERFASSER: D.MAJEWSKI
REAL LAMS,PHIS,POLPHI,POLLAM
DATA ZRPI18 , ZPIR18 / 57.2957795 , 0.0174532925 /
SINPOL = SIN(ZPIR18*POLPHI)
COSPOL = COS(ZPIR18*POLPHI)
ZPHIS = ZPIR18*PHIS
ZLAMS = LAMS
IF(ZLAMS.GT.180.0) ZLAMS = ZLAMS - 360.0
ZLAMS = ZPIR18*ZLAMS
ARG = COSPOL*COS(ZPHIS)*COS(ZLAMS) + SINPOL*SIN(ZPHIS)
PHSTOPH = ZRPI18*ASIN(ARG)
RETURN
END
REAL FUNCTION LMTOLMS (PHI, LAM, POLPHI, POLLAM)
C
C%Z% Modul %M%, V%I% vom %G%, extrahiert am %H%
C
C**** LMTOLMS - FC:UMRECHNUNG DER WAHREN GEOGRAPHISCHEN LAENGE LAM
C**** AUF EINEM PUNKT MIT DEN KOORDINATEN (PHIS, LAMS)
C**** IM ROTIERTEN SYSTEM. DER NORDPOL DES SYSTEMS HAT
C**** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** AUFRUF : LAM = LMTOLMS (PHI, LAM, POLPHI, POLLAM)
C** ENTRIES : KEINE
C** ZWECK : UMRECHNUNG DER WAHREN GEOGRAPHISCHEN LAENGE LAM AUF
C** EINEM PUNKT MIT DEN KOORDINATEN (PHIS, LAMS) IM
C** ROTIERTEN SYSTEM. DER NORDPOL DIESES SYSTEMS HAT
C** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** VERSIONS-
C** DATUM : 03.05.90
C**
C** EXTERNALS: KEINE
C** EINGABE-
C** PARAMETER: PHI REAL BREITE DES PUNKTES IM GEOGR. SYSTEM
C** LAM REAL LAENGE DES PUNKTES IM GEOGR. SYSTEM
C** POLPHI REAL GEOGR.BREITE DES N-POLS DES ROT. SYSTEMS
C** POLLAM REAL GEOGR.LAENGE DES N-POLS DES ROT. SYSTEMS
C** AUSGABE-
C** PARAMETER: WAHRE GEOGRAPHISCHE LAENGE ALS WERT DER FUNKTION
C** ALLE WINKEL IN GRAD (NORDEN>0, OSTEN>0)
C**
C** COMMON-
C** BLOECKE : KEINE
C**
C** FEHLERBE-
C** HANDLUNG : KEINE
C** VERFASSER: G. DE MORSIER
REAL LAM,PHI,POLPHI,POLLAM
DATA ZRPI18 , ZPIR18 / 57.2957795 , 0.0174532925 /
ZSINPOL = SIN(ZPIR18*POLPHI)
ZCOSPOL = COS(ZPIR18*POLPHI)
ZLAMPOL = ZPIR18*POLLAM
ZPHI = ZPIR18*PHI
ZLAM = LAM
IF(ZLAM.GT.180.0) ZLAM = ZLAM - 360.0
ZLAM = ZPIR18*ZLAM
ZARG1 = - SIN(ZLAM-ZLAMPOL)*COS(ZPHI)
ZARG2 = - ZSINPOL*COS(ZPHI)*COS(ZLAM-ZLAMPOL)+ZCOSPOL*SIN(ZPHI)
IF (ABS(ZARG2).LT.1.E-30) THEN
IF (ABS(ZARG1).LT.1.E-30) THEN
LMTOLMS = 0.0
ELSEIF (ZARG1.GT.0.) THEN
LMTOLMS = 90.0
ELSE
LMTOLMS = -90.0
ENDIF
ELSE
LMTOLMS = ZRPI18*ATAN2(ZARG1,ZARG2)
ENDIF
RETURN
END
REAL FUNCTION PHTOPHS (PHI, LAM, POLPHI, POLLAM)
C
C%Z% Modul %M%, V%I% vom %G%, extrahiert am %H%
C
C**** PHTOPHS - FC:UMRECHNUNG DER WAHREN GEOGRAPHISCHEN BREITE PHI
C**** AUF EINEM PUNKT MIT DEN KOORDINATEN (PHIS, LAMS)
C**** IM ROTIERTEN SYSTEM. DER NORDPOL DES SYSTEMS HAT
C**** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** AUFRUF : PHI = PHTOPHS (PHI, LAM, POLPHI, POLLAM)
C** ENTRIES : KEINE
C** ZWECK : UMRECHNUNG DER WAHREN GEOGRAPHISCHEN BREITE PHI AUF
C** EINEM PUNKT MIT DEN KOORDINATEN (PHIS, LAMS) IM
C** ROTIERTEN SYSTEM. DER NORDPOL DIESES SYSTEMS HAT
C** DIE WAHREN KOORDINATEN (POLPHI, POLLAM)
C** VERSIONS-
C** DATUM : 03.05.90
C**
C** EXTERNALS: KEINE
C** EINGABE-
C** PARAMETER: PHI REAL BREITE DES PUNKTES IM GEOGR. SYSTEM
C** LAM REAL LAENGE DES PUNKTES IM GEOGR. SYSTEM
C** POLPHI REAL GEOGR.BREITE DES N-POLS DES ROT. SYSTEMS
C** POLLAM REAL GEOGR.LAENGE DES N-POLS DES ROT. SYSTEMS
C** AUSGABE-
C** PARAMETER: ROTIERTE BREITE PHIS ALS WERT DER FUNKTION
C** ALLE WINKEL IN GRAD (NORDEN>0, OSTEN>0)
C**
C** COMMON-
C** BLOECKE : KEINE
C**
C** FEHLERBE-
C** HANDLUNG : KEINE
C** VERFASSER: G. DE MORSIER
REAL LAM,PHI,POLPHI,POLLAM
DATA ZRPI18 , ZPIR18 / 57.2957795 , 0.0174532925 /
ZSINPOL = SIN(ZPIR18*POLPHI)
ZCOSPOL = COS(ZPIR18*POLPHI)
ZLAMPOL = ZPIR18*POLLAM
ZPHI = ZPIR18*PHI
ZLAM = LAM
IF(ZLAM.GT.180.0) ZLAM = ZLAM - 360.0
ZLAM = ZPIR18*ZLAM
ZARG = ZCOSPOL*COS(ZPHI)*COS(ZLAM-ZLAMPOL) + ZSINPOL*SIN(ZPHI)
PHTOPHS = ZRPI18*ASIN(ZARG)
RETURN
END
c ------------------------------------------------------------------
c Compute Cos/Sin of an argument in Degree instead of Radian
c ------------------------------------------------------------------
real function cosd(arg)
real,intent(IN) :: arg
real,parameter :: grad2rad=3.1415926/360.
cosd=cos(arg*grad2rad)
return
end
real function sind(arg)
real,intent(IN) :: arg
real,parameter :: grad2rad=3.1415926/360.
sind=sin(arg*grad2rad)
return
end