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nmsyn2.f90
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program spherical
!
implicit none
!
include "spherical.h"
!
include "minos.h"
!
integer yr,jda,ho,mi
integer yr1,jda1,ho1,mi1
integer ns,nps,nstn
integer i,j,ios,iom
integer is,ir
integer lnblnk
integer n,l,lprev
real elat,elon,depth
real sphif,sdlt,slnda,moment
real mrr,mtt,mpp,mrt,mrp,mtp
real radius,rho,vpv,vph,vsv,vsh,eta,qmu,qkappa
real r(NL)
real rs,ws,dws,us,dus,vs,dvs
real w(NL),dw(NL)
real u(NL),du(NL),v(NL),dv(NL)
real rlat,rlon,stele,stbur,stazi,stdip,spsec,sec1
double precision delta,aze,azr
double precision k,fac
double precision a0,a1,a2,b1,b2
double precision a,dadt,dadp
double precision amp(3)
double precision t0,ts,dt,hdur,reclen
double precision theta,phi
double precision om,q,av,ah
double precision sint,cost,p(3),dp(3)
double precision sinp,cosp,sin2p,cos2p
double precision T_min,T_max,om_min,om_max
double precision seismogram(3,NTMAX)
character(len=250) :: inp_fname
character(len=4 ) :: stn
character(len=2 ) :: ntw
character(len=80 ) :: cmt_file,station_file
character(len=80 ) :: model_file,toroidal_file,radial_file,spheroidal_file
! read main input file
! get input file name
call get_command_argument(1, inp_fname)
! open file to read
open(unit=11,file=trim(inp_fname),status='old', action='read',iostat=ios)
if (ios /= 0)then
write(*,'(a)')'ERROR: input file "'//trim(inp_fname)//&
'" cannot be opened!'
return
endif
! specify the catalogue information
read(11,'(a)') model_file
read(11,'(a)') toroidal_file
read(11,'(a)') radial_file
read(11,'(a)') spheroidal_file
print *,' '
print *,' model file: ',model_file(1:lnblnk(model_file))
print *,' toroidal mode file: ',toroidal_file(1:lnblnk(toroidal_file))
print *,' radial mode file: ',radial_file(1:lnblnk(radial_file))
print *,'spheroidal mode file: ',spheroidal_file(1:lnblnk(spheroidal_file))
! specify cmtsolution file name
read(11,'(a)') cmt_file
print *,' '
print *,' CMTSOLUTION file: ',cmt_file(1:lnblnk(cmt_file))
call get_cmt(cmt_file,yr,jda,ho,mi,sec,t_cmt,hdr,elat,elon,depth,mrr,mtt, &
mpp,mrt,mrp,mtp)
hdur=dble(hdr)
read(11,'(a)') station_file
print *,' '
print *,' STATION file: ',station_file(1:lnblnk(station_file))
! specify the shortest period in mode summation
read(11,*) T_min
T_max=6000.0d0
om_max=PI2/T_min
om_min=PI2/T_max
print *,' '
print *,'shortest period in mode sum: ',T_min,' seconds'
! specify sampliing rate and length of the record in seconds
read(11,*) dt,reclen
close(11)
if (2*dt > T_min) stop ' Sampling rate too large'
nps=int(reclen/dt)
t0=0.0
print *,' '
print *,'start time (s): ',t0, ' dt (s): ',dt
print *,'record length (s): ', reclen,' npts: ',nps
! get the radii for the upper NL layers at which the eigenfunctions
! are stored; needed for source radius
open(unit=1,file=trim(model_file))
rewind(1)
j=0
do i=1,NR
read(1,*) ir,radius,rho,vpv,vph,vsv,vsh
if(i.gt.NR-NL) then
j=j+1
r(j)=radius/RA
endif
enddo
close(unit=1)
if(j.ne.NL) call exit(1)
! get the source radius and index
!
rs=1.0-depth*1000.0/RA ! non-dimensionalized source radius
is=NL
do while(r(is).gt.rs) ! find radius r(is) just below source radius rs
is=is-1
enddo
if(is.lt.1) call exit(1)
!
! read the station information and loop over stations
!
open(unit=1,file=trim(station_file),status='old',iostat=ios)
if (ios.ne.0) stop 'Error opening station file STATIONS'
read(1,*,iostat=ios) nstn
print *,' '
print *,'number of stations: ', nstn
read(1,*,iostat=ios) stn,ntw,rlat,rlon,stele,stbur
do while (ios .eq. 0)
ns=1
ts=t0
!
! epicentral distance and azimuth
!
call delaz(elat,elon,rlat,rlon,delta,aze,azr)
!
print *,' '
print *,'station: ',stn(1:lnblnk(stn))
print *,'epicentral distance: ',delta,' degrees'
!
! aze is measured clockwise from due North by delaz; convert this
! to a counterclockwise measurement from due South, which is the
! Dahlen & Tromp convention
!
aze=180.0d0-aze
if(aze.lt.0.0d0) aze=aze+360.0d0
print *,'source azimuth: ',aze,' degrees (c.c. from due South)'
!
! initialize information for Legendre calculations
!
theta=delta*PI/180.0d0
sint=dsin(theta)
if(sint.lt.1.0d-09) sint=1.0d-09
cost=dcos(theta)
phi=aze*PI/180.0d0
sinp=dsin(phi)
cosp=dcos(phi)
sin2p=dsin(2.0d0*phi)
cos2p=dcos(2.0d0*phi)
!
! initialize the three-component mode sum
!
do i=1,nps
do j=1,3
seismogram(j,i)=0.0d0
enddo
enddo
print *,' '
print *,'Start mode summation ....'
!
! start toroidal mode sum
!
open(unit=2,file=trim(toroidal_file),status='old',form='unformatted')
rewind(2)
iom=0
lprev=0
do while(iom.eq.0)
read(2,iostat=iom)n,l,om,q,av,ah,(w(i),i=1,NL),(dw(i),i=1,NL)
if(iom.eq.0) then
if(om.ge.om_min.and.om.le.om_max) then
! minos calculates and stores all the overtones for a give
! degree, so Legendre polynomials have to be calculated
! only once per degree
!
if(l.ne.lprev) then
call plm(l,cost,sint,p,dp)
k=dsqrt(dble(l*(l+1)))
fac=dble(2*l+1)/(4.0d0*PI)
lprev=l
endif
!
! get w and dw at the source radius rs
!
if(r(is).eq.rs) then
ws=w(is)
dws=dw(is)
else
call interpolate(r(is),w(is),dw(is),r(is+1),w(is+1),dw(is+1),rs,ws,dws)
endif
!
! Dahlen & Tromp (10.56-10.59) for toroidal modes,
! but with minos modes: W_DT=om*W_minos
!
a1=dble(-mrp*(dws-ws/rs)/k)
b1=dble(mrt*(dws-ws/rs)/k)
a2=dble(-mtp*ws/(k*rs))
b2=dble(0.5*(mtt-mpp)*ws/(k*rs))
!
dadt=dp(2)*(a1*cosp+b1*sinp)+dp(3)*(a2*cos2p+b2*sin2p)
dadp=p(2)*(-a1*sinp+b1*cosp)+2.0d0*p(3)*(-a2*sin2p+b2*cos2p)
!
! longitudinal and transverse components
!
amp(1)=0.0d0 !vertical
amp(2)=fac*ah*dadp/sint !longitudinal
amp(3)=-fac*ah*dadt !transverse
!
call time_series(ns,ts,nps,dt,om,q,hdur,amp,seismogram)
!
endif
endif
enddo
close(unit=2)
print *,'Finishing toroidal modes....'
!
! start radial mode sum
!
open(unit=2,file=trim(radial_file),status='old',form='unformatted')
rewind(2)
iom=0
do while(iom.eq.0)
read(2,iostat=iom)n,l,om,q,av,ah,(u(i),i=1,NL),(du(i),i=1,NL)
if(iom.eq.0) then
if(om.ge.om_min.and.om.le.om_max) then
if(n.eq.0) then
fac=1.0d0/(4.0d0*PI)
p(1)=1.0d0
endif
!
! get u and du at the source radius rs
!
if(r(is).eq.rs) then
us=u(is)
dus=du(is)
else
call interpolate(r(is),u(is),du(is),r(is+1),u(is+1),du(is+1), &
rs,us,dus)
endif
!
! Dahlen & Tromp (10.54) for radial modes,
! but with minos modes: U_DT=om*U_minos
!
a0=dble(mrr*dus+(mtt+mpp)*us/rs)
!
a=p(1)*a0
!
! vertical component
!
amp(1)=fac*av*a
amp(2)=0.0d0
amp(3)=0.0d0
!
call time_series(ns,ts,nps,dt,om,q,hdur,amp,seismogram)
!
endif
endif
enddo
close(unit=2)
print *,'Finishing radial modes....'
!
! start spheroidal mode sum
!
open(unit=2,file=trim(spheroidal_file),status='old',form='unformatted')
rewind(2)
iom=0
lprev=0
do while(iom.eq.0)
read(2,iostat=iom)n,l,om,q,av,ah,(u(i),i=1,NL),(du(i),i=1,NL), &
(v(i),i=1,NL),(dv(i),i=1,NL)
if(iom.eq.0) then
if(om.ge.om_min.and.om.le.om_max) then
if(l.ne.lprev) then
call plm(l,cost,sint,p,dp)
k=dsqrt(dble(l*(l+1)))
fac=dble(2*l+1)/(4.0d0*PI)
lprev=l
endif
!
! get u, du, v, and dv at the source radius rs
!
if(r(is).eq.rs) then
us=u(is)
dus=du(is)
vs=v(is)
dvs=dv(is)
else
call interpolate(r(is),u(is),du(is),r(is+1),u(is+1),du(is+1), &
rs,us,dus)
call interpolate(r(is),v(is),dv(is),r(is+1),v(is+1),dv(is+1), &
rs,vs,dvs)
endif
!
! Dahlen & Tromp (10.54-10.59) for spheroidal modes,
! with U_DT=om*U_minos and V_DT=om*V_minos
!
a0=dble(mrr*dus+(mtt+mpp)*(us-0.5*k*vs)/rs)
a1=dble(mrt*(dvs-vs/rs+k*us/rs)/k)
b1=dble(mrp*(dvs-vs/rs+k*us/rs)/k)
a2=dble(0.5*(mtt-mpp)*vs/(k*rs))
b2=dble(mtp*vs/(k*rs))
!
a=p(1)*a0+p(2)*(a1*cosp+b1*sinp)+p(3)*(a2*cos2p+b2*sin2p)
dadt=dp(1)*a0+dp(2)*(a1*cosp+b1*sinp)+dp(3)*(a2*cos2p+b2*sin2p)
dadp=p(2)*(-a1*sinp+b1*cosp)+2.0d0*p(3)*(-a2*sin2p+b2*cos2p)
!
! vertical, longitudinal, and transverse components
!
amp(1)=fac*av*a !vertical
amp(2)=fac*ah*dadt !longitudinal
amp(3)=fac*ah*dadp/sint !transverse
!
call time_series(ns,ts,nps,dt,om,q,hdur,amp,seismogram)
!
endif
endif
enddo
close(unit=2)
print *,'Finishing spheroidal modes....'
call write_record(elat,elon,rlat,rlon,stn,ntw,dt,nps,seismogram)
!
read(1,*,iostat=ios) stn,ntw,rlat,rlon,stele,stbur
enddo
close(1)
!
print *,' '
print *,' DONE '
print *,' '
!
end program spherical
!===============================================================================
subroutine interpolate(r1,f1,df1,r2,f2,df2,rs,fs,dfs)
!
implicit none
!
! interpolate finds the value of a function fs and its derivative dfs
! at the radius rs by interpolating given values of the function and its
! derivative just below the source at radius r1, given by f1 and df1,
! and values just above the source ar radius r2, given by f2 and df2.
! Note that we should have r2 > rs > r1.
!
real r1,f1,df1,r2,f2,df2,rs,fs,dfs
!
real h,dr
!
h=rs-r1
dr=r2-r1
if((h.lt.0.0).or.(dr.lt.0.0)) then
write(6,"('wrong input in interpolate')")
call exit(1)
endif
!
fs=f1+h*df1+0.5*h*h*(df2-df1)/dr
dfs=df1+h*(df2-df1)/dr
return
end subroutine interpolate
!===============================================================================