Skip to content

O
OpenFlatus
Commit a56b9e68 authored by Matheus Müller's avatar Matheus Müller
Browse files
Options

Implementado modelo monocamadas 

Lento - sugerido multithread para acelerar
parent d8775ca1
Expand all Hide whitespace changes
Inline Side-by-side
Showing with 5120 additions and 5092 deletions
calc.py
View file @ a56b9e68
......@@ -24,6 +24,11 @@ def kinematic(mt, mi, esp):
MM = mi/mt
return ((sqrt (1. - MM**2.*sin(esp)**2.) + MM*cos(esp) ) / (1. + MM) )**2.
####################################################################################################################################################
# Coeficientes de Poisson
def kpoisson(n, m, x):
return (m*x)**n*exp(-m*x)/math.factorial(n)
####################################################################################################################################################
# Funcoes em comum
......@@ -146,10 +151,13 @@ def calc(p, modelo, ion, OFlabentries, LScontrol, CGausscontrol, metodo, espectr
def spectrolayer(p, modelo, ion, OFlabentries, LScontrol, CGausscontrol, metodo, espectro, emin, plote, fig, firsttime, botoes, indice, aux, aux2):
EPasso, passox, e, resol, dose, Emin, Emax = variables(OFlabentries)
passox = 0.005
gshift=0.
curdepht=passox #Avoid zero division
espectro.clear()
espectro.spectro[0] = 1.
aux.clear()
aux2.clear()
aux2.spectro[0] = 1./EPasso
Theta_s = PI - (p['Theta_in'] + p['Theta_out'])*PI/180.
mi = ion['mass']
......@@ -170,9 +178,6 @@ def spectrolayer(p, modelo, ion, OFlabentries, LScontrol, CGausscontrol, metodo,
k = ((sqrt (mt**2.-mi**2.*(sin(Theta_s)**2.)) + mi*cos(Theta_s) ) / (mi+mt) )**2.
dedxef=dedx*(k/cos(p['Theta_in']*PI/180.) + 1./cos(p['Theta_out']*PI/180.))
dw2dxef=dW2dx*(k**2./cos(p['Theta_in']*PI/180.)+1./cos(p['Theta_out']*PI/180.))
sinalbessel = e*0.
sinalgaussiana = e*0.
# Calcula a contribuição de cada passo
for x in arange(curdepht, xfinal, passox):
......@@ -181,41 +186,31 @@ def spectrolayer(p, modelo, ion, OFlabentries, LScontrol, CGausscontrol, metodo,
CS = c*k*CSRf(ion['Z'], camada.Elements[componente]['Z'], k*p['E0']-dedxef*x, mi, mt, Theta_s)*passox
# É multiplicada pelo passo para manter a escala do gráfico independente do mesmo.
# Bessel:
if modelo == 'bessel':
alpha=dedxef*(2./dw2dxef)
m=alpha*dedxef
lbd=m*x*alpha
a = ((p['E0'] - k*dedxef)/p['E0'])
aux.clear()
aux.spectro[0] = a*1./EPasso #[int((k*p['E0'])/EPasso-1)] = exp(-m*x)+x*m*alpha*exp(-m*x)*i1(0)/sqrt(0.00000000001)*passox*passox
#lbd*exp(-m*x-alpha*(k*p['E0']-e))*i1(2.*sqrt(lbd*(k*p['E0']-e)))/(sqrt(lbd*(k*p['E0']-e)+.0000001))
aux.soma( alpha*exp(-alpha*arange(0,10.,passox)*dedxef))
espectro.Convolve(aux)
#espectro.soma(aux2.spectro*CS)
alpha=dedxef*(2./dw2dxef)
m=alpha*dedxef
# Gaussiana:
elif modelo == 'gaussiana':
Em=k*p['E0']-x*dedxef
sigma=x*dw2dxef
gaussianacamada = exp((-(e-Em)**2.)/(2.*sigma))/sqrt(2.*PI*sigma)
espectro.soma( list(nan_to_num(gaussianacamada*CS)) )
if modelo == 'bessel':
linecolor='r'
aux.clear()
for y in range(20):
aux.soma(kpoisson((y+1.),m,passox)*alpha*exp(-alpha*aux.axisenergy()))
aux.spectro[0] = kpoisson(0.,m,passox)*1./EPasso
elif modelo == 'gaussiana':
linecolor='b'
aux2.Convolve(aux)
aux2.multiply(CS)
espectro.soma(aux2.spectro)
aux2.multiply(1./CS)
linecolor='b'
curdepht = xfinal
espectro.reverse()
if LScontrol == 1:
espectro.ConvolveF0(1./alpha_lineshape)
if CGausscontrol == 1:
espectro.ConvolveGauss(resol/2.35482)
espectro.multiply(dose)
espectro.spectro[0]=0.
espectro.eshift = espectro.eshift - (1-k)*p['E0'] - EPasso
espectro.multiply(dose*0.93)
plote[indice].set_xdata(espectro.axisenergy())
plote[indice].set_ydata(espectro.spectro)
......
script.py
View file @ a56b9e68
......@@ -7,6 +7,9 @@ espectro2 = spectro(2000, 50)
espectro3 = spectro(2000, 50)
espectro2.spectro[0] = 1.
def k(n, m, x):
return (m*x)**n*exp(-m*x)/math.factorial(n)
def CSRf(Z1, Z2, Ein, M1, M2, Theta):
if M1 < M2:
return ((Z1*Z2*4.8e-20*1.e8)/(4.*Ein))**2. * sin(Theta)**-4.
......@@ -14,8 +17,7 @@ def CSRf(Z1, Z2, Ein, M1, M2, Theta):
return 0.
x = arange(0,1.,0.05)
k = 1.
x = arange(0,1.,0.01)
dedx = 250.
dW2dx = 26500.
mt=178.
......@@ -23,26 +25,48 @@ mi=1.
Theta_in = 0.
Theta_out = 70.
Theta_s = PI - (Theta_in + Theta_out)*PI/180.
k = ((sqrt (mt**2-mi**2*(sin(Theta_s)**2)) + mi*cos(Theta_s) ) / (mi+mt) )**2
dedxef=dedx*(k/cos(Theta_in*PI/180.) + 1./cos(Theta_out*PI/180.))
dw2dxef=dW2dx*(k**2./cos(Theta_in*PI/180.)+1./cos(Theta_out*PI/180.))
kc = ((sqrt (mt**2-mi**2*(sin(Theta_s)**2)) + mi*cos(Theta_s) ) / (mi+mt) )**2
dedxef=dedx*(kc/cos(Theta_in*PI/180.) + 1./cos(Theta_out*PI/180.))
dw2dxef=dW2dx*(kc**2./cos(Theta_in*PI/180.)+1./cos(Theta_out*PI/180.))
alpha=dedxef*(2./dw2dxef)
E0 = 100000.
m=alpha*dedxef
for j in x:
CS = k*CSRf(1., 72., k*E0-dedxef*j, mi, mt, Theta_s)*0.05
a = ((E0 - 2*k*dedxef)/E0)
CS = kc*CSRf(1., 72., kc*E0-dedxef*j, mi, mt, Theta_s)*0.05
a = k(0.,m,0.01)
b = k(1.,m,0.01)
c = k(2.,m,0.01)
d = k(3.,m,0.01)
e = k(4.,m,0.01)
f = k(5.,m,0.01)
espectro.clear()
espectro.soma(CS*alpha*exp(-alpha*x*dedxef))
espectro.spectro[0] = CS*a*1./50. #- espectro.norma() #espectro.spectro[0] + (1.-espectro.norma())/50.
espectro.spectro[0] = a*1./50.
espectro.soma(b*alpha*exp(-alpha*espectro.axisenergy()))
espectro.soma(c*alpha*exp(-alpha*espectro.axisenergy()))
espectro.soma(d*alpha*exp(-alpha*espectro.axisenergy()))
espectro.soma(e*alpha*exp(-alpha*espectro.axisenergy()))
espectro.soma(f*alpha*exp(-alpha*espectro.axisenergy()))
espectro2.Convolve(espectro)
espectro2.multiply(CS)
espectro3.soma(espectro2.spectro)
espectro2.multiply(1./CS)
#print '#',int(j/0.05), ' Area ',' Media ','Variancia ','\nkmda', espectro2.norma(), espectro2.firstmoment(), espectro2.secondmoment()
#print 'conv', espectro2.norma(), espectro2.firstmoment(), espectro2.secondmoment()
#print 'soma', espectro3.norma(), espectro3.firstmoment(), espectro3.secondmoment(), '\n'
espectro3.reverse()
espectro3.ConvolveF0(1./200.)
espectro3.ConvolveGauss(250./2.35482)
#plot(espectro2.axisenergy(),espectro2.spectro)
espectro3.multiply(22.e33)
#espectro3.eshift = espectro3.eshift - 1600.
plot(espectro3.axisenergy(),espectro3.spectro)
#plot(espectro3.axisenergy(),espectro3.reverse())
espectro2.multiply(99000.)
plot(espectro2.axisenergy(),espectro2.reverse())
amostra = np.loadtxt('monoteste.sim')
xxx= amostra[:,0]*1000
ccc=amostra[:,1]
......
spec.py
View file @ a56b9e68
......@@ -19,7 +19,7 @@ class spectro:
self.size = N ### Tamanho do Vetor ###
def norma(self): ### Retorna a area total do espectro ###
return sum(self.spectro)/self.stepsize
return sum(self.spectro)*self.stepsize
def axisenergy(self): ### Retorna o vetor com as energias analogas a self.spectro ###
ae = arange(self.eshift,((self.size*self.stepsize)+self.eshift-1),self.stepsize)
......@@ -44,7 +44,7 @@ class spectro:
temp = list()
for j in range(self.size):
temp.insert(j, self.spectro[int(self.size-j-1)])
return temp
self.spectro = temp
def multiply(self, factor): ### Multiplica o espectro por um fator ###
for j in range(self.size):
......@@ -93,16 +93,25 @@ class spectro:
self.normalize()
def firstmoment(self): ### Retorna o primeiro momento da distribuicao ###
moment=0;
for i in arange(0,self.size,1):
moment = moment + (1.*i*self.stepsize)*self.spectro[i]
return moment/self.norma()
moment=0.;
i=0;
#for i in arange(0,self.size,1):
# moment = moment + (1.*i*self.stepsize)*self.spectro[i]
while moment < self.norma()/2.:
moment = moment +self.spectro[i]*self.stepsize
i= i +1
return i*self.stepsize
def secondmoment(self): ### Retorna o segundo momento da distribuicao ###
moment=0;
for i in arange(0,self.size,1):
moment = moment + (1.*i*self.stepsize)**2*self.spectro[i]
return moment/self.norma()
#a = list()
#for k in range(self.size):
# a.insert(k, [self.axisenergy()[k],self.spectro[k]])
#return np.var(a)#
return moment/self.norma()
#print self.axisenergy()
def thirdmoment(self): ### Retorna o terceiro momento da distribuicao ###
moment=0;
......
temp.sim
View file @ a56b9e68
This diff is collapsed.
Markdown is supported
0% or
You are about to add 0 people to the discussion. Proceed with caution.
Finish editing this message first!
Please register or to comment