Currently prints range values to terminal. I need to export these values to a csv file. "print S[t-1], I[t-1], R[t-1]" are the values...
import matplotlib.pyplot as plt
import numpy
beta = 0.24
gamma = 0.142857
Tstart = 0
Tend = 151
r = 0
s = (306.8 * 10**6)
i = (22 * 10**6)
def compute_next_day(t,R,I,S):
R[t] = gamma * I[t - 1] + R[t - 1]
I[t] = (beta * I[t-1] * S[t-1] / (r+i+s)) - gamma * I[t-1] + I[t-1]
S[t] = - (beta * I[t-1] * S[t-1] / (r+i+s)) + S[t-1]
print S[t-1], I[t-1], R[t-1]
def compute_entire_period(Tstart, Tend, R, I, S):
R[Tstart] = r
I[Tstart] = i
S[Tstart] = s
for t in range(Tstart + 1, Tend):
compute_next_day(t, R, I, S)
R = range(Tstart, Tend)
I = range(Tstart, Tend)
S = range(Tstart, Tend)
If you want to save data in a CSV, use the dsv library:
import csv
beta = 0.24
gamma = 0.142857
Tstart = 0
Tend = 151
r = 0
s = (306.8 * 10 ** 6)
i = (22 * 10 ** 6)
def compute_next_day(t, R, I, S):
R[t] = gamma * I[t - 1] + R[t - 1]
I[t] = (beta * I[t - 1] * S[t - 1] / (r + i + s)) - gamma * I[t - 1] + I[t - 1]
S[t] = - (beta * I[t - 1] * S[t - 1] / (r + i + s)) + S[t - 1]
return [S[t-1], I[t-1], R[t-1]]
def compute_entire_period(Tstart, Tend, R, I, S):
R[Tstart] = r
I[Tstart] = i
S[Tstart] = s
with open('mydata.csv', 'w') as mycsvfile:
writer = csv.writer(mycsvfile)
for t in range(Tstart + 1, Tend):
writer.writerow(compute_next_day(t, R, I, S))
R = range(Tstart, Tend)
I = range(Tstart, Tend)
S = range(Tstart, Tend)
compute_entire_period(Tstart, Tend, R, I, S)
Something like this should work:
def compute_next_day(t,R,I,S,):
...
return S[t-1], I[t-1], R[t-1] # return values instead of printing to terminal
with open('path_to_file.csv','w') as f:
for ... : # your choice of loop
vals = compute_next_day(...) # compute your values
f.write(','.join(vals) + '\n') # dump your values separated with ','
Related
I am trying to make several plots for a project of mine using the following code:
import pprint
import scipy
import scipy.linalg # SciPy Linear Algebra Library
import numpy as np
from scipy.linalg import lu , lu_factor, lu_solve
from scipy.integrate import quad
import matplotlib.pyplot as plt
#Solving the equations for the Prandtl case
K = 100
alpha = 0.1
visc = 5
diff = 5
N = 0.01
L = 5000
height = 250
subdivisions = 100
tick = 10
points = np.arange(0,L/2+tick,tick)
def H(y):
return ( height * (1 + np.cos(2 * np.pi * y/L)) )
def Bsfc(y):
return 0.1
final_system = []
b=[]
for q in range(-K,K+1):
equation1 = []
equation2 = []
equation3 = []
Aki = []
Cki = []
Dki = []
for k in range(-K,K+1):
R = 2 * N**2 * np.cos(alpha)**2 / (visc * diff) * (k * np.pi / L)**2
Q = N**2 * np.sin(alpha)**2 / (3 * visc * diff)
S1 = abs(R + np.sqrt(Q**3 + R**2) )**(1/3)
S2 = - abs( np.sqrt(Q**3 + R**2) -R )**(1/3)
phi = np.sqrt(S1**2 + S2**2 - S1*S2)
Lk = np.arccos(- (S1 + S2)/ (2 * phi) )
m1 = - np.sqrt(S1 + S2)
m2 = - np.sqrt(phi) * np.exp(1j * Lk/2)
m3 = m2.conjugate()
def f1r(y):
return (np.exp(m1 * H(y)) * np.cos(2 * (q - k) * np.pi * y / L) ).real
def f1i(y):
return (np.exp(m1 * H(y)) * np.cos(2 * (q - k) * np.pi * y / L) ).imag
gamma1 = 2/L * (quad(f1r,0,L/2,limit=subdivisions)[0] + quad(f1i,0,L/2,limit=subdivisions)[0]*1j)
def f2r(y):
return (np.exp(m2 * H(y)) * np.cos(2 * (q - k) * np.pi * y / L) ).real
def f2i(y):
return (np.exp(m2 * H(y)) * np.cos(2 * (q - k) * np.pi * y / L) ).imag
gamma2 = 2/L * (quad(f2r,0,L/2,limit=subdivisions)[0] + quad(f2i,0,L/2,limit=subdivisions)[0]*1j)
if k == 0:
equation1.append(2 * gamma2.real)
Cki.append(k)
equation1.append(-2 * gamma2.imag)
Dki.append(k)
else:
equation1.append(gamma1)
Aki.append(k)
equation1.append(2 * gamma2.real)
Cki.append(k)
equation1.append(-2 * gamma2.imag)
Dki.append(k)
if q != 0:
if k == 0:
equation2.append(0)
equation2.append(0)
else:
equation2.append(k * gamma1 / (m1**3) )
equation2.append(2 * k * (gamma2 / (m2**3) ).real)
equation2.append(-2 * k * (gamma2 / (m2**3) ).imag)
if k == 0:
equation3.append(2 * (m2**2 * gamma2).real)
equation3.append(-2 * (m2**2 * gamma2).imag)
else:
equation3.append(m1**2 * gamma1)
equation3.append(2 * (m2**2 * gamma2).real)
equation3.append(-2 * (m2**2 * gamma2).imag)
final_system.append(equation1)
def f4r(y):
return (Bsfc(y) * np.cos(2 * q * np.pi * y / L) ).real
def f4i(y):
return (Bsfc(y) * np.cos(2 * q * np.pi * y / L) ).imag
b.append(2/L * (quad(f4r,0,L/2,limit=subdivisions)[0] + quad(f4i,0,L/2,limit=subdivisions)[0]*1j))
if q != 0:
final_system.append(equation2)
b.append(0)
final_system.append(equation3)
b.append(0)
final_system = np.array(final_system)
b=np.array(b)
#LU solver
P, Ls, U = scipy.linalg.lu(final_system)
Bl = np.linalg.inv(P) # b
Z = np.linalg.solve(Ls,Bl)
X = np.linalg.solve(U,Z)
print (np.allclose(final_system # X, b))
#Getting the values for Ak, Ck and Dk
strings = []
for k in range(-K,K+1):
if k != 0:
strings.append('A')
strings.append('R')
strings.append('I')
Ak = []
Rk = []
Ik = []
for k in range(0,len(X)):
if 'A' in strings[k]:
Ak.append(X[k])
if 'R' in strings[k]:
Rk.append(X[k])
if 'I' in strings[k]:
Ik.append(X[k])
Ck=[]
for k in range(0,len(Rk)):
Ck.append(Rk[k] + Ik[k] * 1j)
Ck = np.array(Ck)
Dk = Ck.conjugate()
Ak = np.array(Ak)
#Getting the Buoyancy value
z = np.arange(0,2010,10)
y = np.arange(-L,L+10,10)
Y,Z = np.meshgrid(y,z)
B = np.ones_like(Y)*[0]
for k in range(-K,K+1):
R = 2 * N**2 * np.cos(alpha)**2 / (visc * diff) * (k * np.pi / L)**2
Q = N**2 * np.sin(alpha)**2 / (3 * visc * diff)
S1 = abs(R + np.sqrt(Q**3 + R**2) )**(1/3)
S2 = - abs( np.sqrt(Q**3 + R**2) -R )**(1/3)
phi = np.sqrt(S1**2 + S2**2 - S1*S2)
Lk = np.arccos(- (S1 + S2)/ (2 * phi) )
m1 = - np.sqrt(S1 + S2)
m2 = -np.sqrt(phi) * np.exp(1j * Lk/2)
m3 = m2.conjugate()
if k != 0:
B = B + ( Ak[Aki.index(k)] * np.exp(m1 * Z) * np.exp(2j * (k) * np.pi * Y / L) )
B = B + ( ( Ck[Cki.index(k)] * np.exp(m2 * Z) + Dk[Dki.index(k)] * np.exp(m3 * Z) ) * np.exp(2j * (k) * np.pi * Y / L) )
for k in range(0,B.shape[0]):
for t in range(0,B.shape[1]):
if Z[k][t] < H(Y[k][t]):
B[k][t] = np.nan
if Z[k][t] == H(Y[k][t]):
print (B[k][t], "B value at the ground")
if abs(Z[k][t] - H(Y[k][t])) < 0.1:
if B[k][t] > 0.101:
print (B[k][t],'error -------------------------------------------------')
# print (B[k][t], Z[k][t], H(Y[k][t]), Y[k][t], '-----------------------------------------------------------------------------' )
Bp = Bsfc(Y) * np.exp(-Z * np.sqrt(N * np.sin(alpha) ) / (4*visc*diff)**(1/4) ) * np.cos(np.sqrt(N*np.sin(alpha)) /((4*visc*diff)**(1/4))*Z )
##Plotting the buoyancy
fig = plt.figure(figsize=(10,10)) # create a figure
plt.rcParams.update({'font.size':16})
plt.title('Buoyancy')
plt.contourf(Y,Z,B,np.arange(-0.2,0.201,0.001),cmap='seismic')
#plt.contourf(Y,Z,B,cmap='seismic')
plt.colorbar(label='1/s')
plt.xlabel("Y axis")
plt.ylabel("Height")
plt.xlim([-L,L])
plt.ylim([0,1500])
plt.show()
The following plot shows a run that yielded a good result:
Buoyancy
However, when I increase the "height" parameter, I start getting unstable results, which I suspect occurs because of numerical instabilities:
Buoyancy unstable
Is there a way to increase numerical precision in python? I have experimented a bit with numpy.double, but with unsuccessful results so far.
Thanks
I guess you'll find your answer here on Stackoverflow
In the standard library, the decimal module may be what you're looking
for. Also, I have found mpmath to be quite helpful...
I have code that looks like this:
n = 2
disc_weights = np.random.uniform(0, 2 * np.pi, 4*n)
phi = (disc_weights[0] * QubitOperator('X0') +
disc_weights[1] * QubitOperator('Y0') +
disc_weights[2] * QubitOperator('Z0') +
disc_weights[3] * QubitOperator('X1') +
disc_weights[4] * QubitOperator('Y1') +
disc_weights[5] * QubitOperator('Z1') +
disc_weights[6] * QubitOperator('') +
disc_weights[7] * QubitOperator('') )
where QubitOperator is a command in a package I am using. How can I automate this to iterate over X, Y, Z, , 1, 2...n and create phi?
This somewhat does the trick but not quite there yet
phi= functools.reduce(operator.add, (1 * QubitOperator(f'{a}{n}') for a,n in itertools.product(["X", "Y", "Z"], range(n))))
n = 2
disc_weights = np.random.uniform(0, 2 * np.pi, 4*n)
iter_ = itertools.product('XYZ', range(n))
tuple_wrapper = lambda t: f'{t[0]}{t[1]}'
sum_ = 0.0 * QubitOperator('')
for dw in disc_weights:
try:
sum_ += dw * QubitOperator(tuple_wrapper(next(iter_)))
except StopIteration:
sum_ += dw * QubitOperator('')
I am trying to solve a PDE using odeint and the method of lines. My code is definitely wrong - and I'm trying to figure out where it is going wrong.
I am calling the ode solver using odeint(odefunc,y0,tspan) where tspan = np.linspace(0.0, 0.5, 5) & y0 = 1.0*np.ones(3).
I tried printing t within odefunc and am confused by the output. Despite the fact that I am solving up to t=0.5, the last t-value to print is 0.015081203121127767. The number of outputs matches tspan, but I cannot see how it could possibly be solving up to t = 0.5 when the last time in the de function is 0.015. What am I missing?
My DE is time dependent - so this is making it very hard to figure out where things are going wrong because I don't seem to be seeing the times where everything fails.
ETA - this is failing, but running this without some of the irrelevant stuff I am getting the warning ODEintWarning: Excess work done on this call (perhaps wrong Dfun type). Run with full_output = 1 to get quantitative information., which I'm assuming is part of the issue - but it doesn't appear to be halting the code.
MWE
import numpy as np
from scipy.integrate import odeint
import matplotlib.pyplot as plt
import math
import sys
plt.interactive(False)
sigma = 2320
rho = 1000
gravity = 9.81 # [m/s^2]
g = gravity*3600*3600 # [m/hour^2]
S = 0.01
settlingVelocity = 0.02 # [m/s]
ws = settlingVelocity*3600 # [m/hour]
n = 0.04 # [SI]
J = 400 # [Ws/m]
k = 0.02
Cstar = 0.2 * sigma # [kg/m^3]
W = 2 # [m]
D0 = 1.2
Lw = 20
L = 100
tend = 0.5 # in hours
tspan = np.linspace(0.0, tend, 5)
def d(t): # metres
if t < 50: # hours
return 0.5
else:
return 0.05
def Q(t):
return 3600 * (math.sqrt(S)/n)*((W*d(t))**(5/3))/((2*d(t) + W)**(2/3))
def h(t):
return d(t)/2
def beta(t):
return (sigma - rho) * g * h(t)/sigma
def Omega(t):
return rho * g * S * Q(t) # [W/m]
def PsiTime(t):
return rho * g * Q(t) * (D0 - d(t))/(Lw)
N = 10
X = np.linspace(0, L, N)
delX = L/ (N-1)
def odefunc(y, t):
def zetaEh(t):
return k * (PsiTime(t) + Omega(t)) / (J + beta(t))
def zetaEW(t):
return (2*d(t)/(W + 2*d(t))) * k * Omega(t)/(J + beta(t))
def zetaR(t):
return (W/(W + 2*d(t))) * k*Omega(t)/(beta(t))
def zetaEF(t,i):
return (W/(W + 2*d(t))) * k * Omega(t) / (J + beta(t))
C = y[:N]
M = y[N:]
print("time: ", t)
dCdt = np.zeros(X.shape)
dMdt = np.zeros(X.shape)
dCdt[0] = ( # forward difference for dCdx
-Q(t) / (W*d(t)) * (C[1] - C[0]) / delX
+ (zetaEh(t) / (W * d(t))) * ((Cstar - C[0]) / Cstar)
- (ws * C[0] * (beta(t))) / (d(t) * (J + beta(t)))
)
dMdt[0] = 0
# gully channel
for i in range (1, N-1): # central difference
if M[i] + W *C[i] * ws - zetaR(t) * (Cstar - C[i]) / Cstar < 0:
reMass = M[i] + W * C[i] * ws
dCdt[i] = (
-Q(t) / (W*d(t)) * (C[i+1] - C[i - 1]) / (2*delX)
+ 1 / (W * d(t)) * ((zetaEW(t) + zetaEF(t,i)) * (Cstar - C[i]) / Cstar
+ reMass * (1 - (beta(t))/ (J + beta(t))))
- C[i] * ws/d(t)
)
dMdt[i] = -M[i]
else:
dCdt[i] = (
-Q(t) / (W*d(t)) * (C[i+1] - C[i - 1]) / (2*delX)
+ 1 / (W * d(t)) * (zetaEW(t) + zetaR(t)) * (Cstar - C[i]) / Cstar
- C[i] * ws / d(t)
)
dMdt[i] = W * C[i] * ws - zetaR(t) * (Cstar - C[i]) / Cstar
# Final node - backward difference
if M[N-1] + W * C[N-1] * ws - zetaR(t) * (Cstar - C[N-1]) / Cstar < 0:
reMass = M[N-1] + W * C[N-1] * ws
dCdt[N-1] = (
-Q(t) / (W * d(t)) * (C[N-1] - C[N-2]) / delX
+ 1 / (W * d(t)) * ((zetaEW(t) + zetaEF(t, i)) * (Cstar - C[N-1]) / Cstar
+ reMass * (1 - (beta(t)) / (J + beta(t))))
- C[i] * ws / d(t)
)
dMdt[N-1] = -M[N-1]
else:
dCdt[N-1] = (
-Q(t) / (W * d(t)) * (C[N-2] - C[N - 1]) / delX
+ 1 / (W * d(t)) * (zetaEW(t) + zetaR(t)) * (Cstar - C[N-1]) / Cstar
- C[N-1] * ws / d(t)
)
dMdt[N-1] = W * C[N-1] * ws - zetaR(t) * (Cstar - C[N-1]) / Cstar
dydt = np.ravel([dCdt, dMdt])
return dydt
init_C = 0.0 * np.ones(X.shape)
init_M = 0.0 * np.ones(X.shape)
init= np.ravel([init_C, init_M])
sol = odeint(odefunc, init, tspan)
conc = sol[:, :N]
So the purpose of my code is to use inputted data points to give a gaussian plot distribution. I figured out how to make it work with a double gaussian but I'm having a lot of trouble adding a third. Im not quite sure what I'm doing wrong. 1 of the errors I keep getting is an Index Error saying that the list index is out of range. I would appreciate any help with this.
Heres my code:
from pylab import *
import numpy as np
from numpy import loadtxt
from scipy.optimize import leastsq
from scipy.optimize import least_squares
from scipy.stats import iqr
import math
import matplotlib.pyplot as plt
import sys
matplotlib.rcParams['mathtext.default'] = 'regular'
fitfunc_triple = lambda p, x: np.abs(p[0]) * exp(-0.5 * ((x - p[1]) / p[2]) ** 2) + np.abs(p[3]) * exp(
-0.5 * ((x - p[4]) / p[5]) ** 2) + np.abs(p[6]) * exp(-0.5 * ((x - p[7])/ p[8] **2 ))
fitfunc_double = lambda p, x: np.abs(p[0]) * exp(-0.5 * ((x - p[1]) / p[2]) ** 2) + np.abs(p[3]) * exp(
-0.5 * ((x - p[4]) / p[5]) ** 2)
fitfunc_single = lambda p, x: np.abs(p[0]) * exp(-0.5 * ((x - p[1]) / p[2]) ** 2)
errfunc = lambda p, x, y: (y - fitfunc(p, x))
dataR = np.loadtxt("/Users/Safi/Library/Preferences/PyCharmCE2018.1/scratches/rspecial1385.a2261.dat5", skiprows=0)
RA = dataR[:, 0]
DEC = dataR[:, 1]
VELR = dataR[:, 2]
REDSH = dataR[:, 3]
RADD = dataR[:, 4]
sl = 3E5
zbar = np.mean(REDSH)
vc = zbar * sl
VEL = vc + sl * ((REDSH - zbar) / (1 + zbar))
wdith = 200
iters = 10
sig2 = 500
binN = int(math.ceil((np.max(VEL) - np.min(VEL)) / wdith))
sys.stdout = open(str(wdith) + "_1sigma_" + str(iters) + "_sig2_" + str(sig2) + ".txt", "w")
plt.figure(1)
y, x, _ = plt.hist(VEL, binN, alpha=0.5, label='data')
x = (x[1:] + x[:-1]) / 2 # for len(x)==len(y)
data = np.vstack((x, y)).T
xdata = data[:, 0]
ydata = data[:, 1]
yerr = ydata ** 0.5
init = [10, 69500, 1200, 5, 68000, sig2]
bds = ([0, 66000, 800, 0, 66000, sig2], [50, 70000, 1750, 20, 70000, sig2 + 0.01])
def index_outlier(data):
inter_quart = iqr(data) * 1.5
bd2 = np.percentile(data, 75) + inter_quart
bd1 = np.percentile(data, 25) - inter_quart
index = []
for i in [i for i, x in enumerate(data) if x < bd1 or x > bd2]:
index.append(i)
return (index)
#### Bootstrapping Estimation Function ####
def fit_bootstrap(fitfunc, datax, datay, init, bds, sigma, iterations=iters):
errfunc = lambda p, x, y: (y - fitfunc(p, x))
# Fit first time
pfit = least_squares(errfunc, init, bounds=bds, args=(datax, datay), max_nfev=10000)
model = fitfunc(pfit.x, datax)
residuals = pfit.fun
# Random data sets are generated and fitted
ps = []
for i in range(iterations):
randomdataY = []
for k in range(len(sigma)):
randomDelta = np.random.normal(0., sigma[k], 1)
randomdataY.append(datay[k] + randomDelta)
out = np.concatenate(randomdataY)
randomfit = least_squares(errfunc, init, bounds=bds, args=(datax, out))
ps.append(randomfit.x)
# Removing outliers
# Finding outliers and indexing them
master_list = []
indexed = []
for k in range(len(ps[0])): # 0-6
it = []
for i in range(len(ps)): # 0-1000
it.append(ps[i][k])
master_list.append(it)
# indexed.append(index_outlier(master_list[k]))
# # List of outlier indicies
# flat_list=[item for sublist in indexed for item in sublist]
# no_dups= list(set(flat_list))
# # Removing bad fits
# for k in range(len(master_list)):
# for i in sorted(no_dups,reverse=True):
# del master_list[k][i]
pfit_bootstrap = []
perr_bootstrap = []
for i in master_list:
pfit_bootstrap.append(np.median(i))
perr_pos = np.round(np.percentile(i, 84) - np.median(i), 4)
perr_neg = np.round(np.median(i) - np.percentile(i, 16), 4)
perr_bootstrap.append(str('[+') + str(perr_pos) + str(',-') + str(perr_neg) + str(']'))
return (pfit_bootstrap, perr_bootstrap, residuals, pfit.nfev, master_list)
pfit, perr, residuals, nfev, master_list = fit_bootstrap(fitfunc_double, xdata, ydata, init, bds, yerr)
pfit1, perr1, residuals1, nfev1, master_list1 = fit_bootstrap(fitfunc_single, xdata, ydata, init, bds, yerr)
more_data = np.linspace(np.min(xdata), np.max(xdata), 1000)
real_func = fitfunc_double(pfit, more_data)
real_func1 = fitfunc_single(pfit1, more_data)
######## Saving Coefficients #########
A1 = pfit[0]
m1 = pfit[1]
s1 = pfit[2]
A2 = pfit[3]
m2 = pfit[4]
s2 = pfit[5]
A3 = pfit[6]
m3 = pfit[7]
s3 = pfit[8]
pecp = VEL - vc
m1p = m1 - vc
m2p = m2 - vc
m3p = m3 - vc
xdatap = xdata - vc
plt.figure(6)
plt.hist(pecp, binN, alpha=.5, label='data', color='skyblue')
xhmax = np.amax(pecp + 1500)
xhmin = np.amin(pecp - 1500)
xh = np.linspace(xhmin, xhmax, 50)
# yh1=(mlab.normpdf(xh, c[1], c[2]))
yh1 = np.abs(A1) * exp(-0.5 * (((xh - m1p) / (s1)) ** 2))
yh2 = np.abs(A2) * exp(-0.5 * (((xh - m2p) / (s2)) ** 2))
yh3 = np.abs(A3) * exp(-0.5 * (((xh - m3p) / (s3)) ** 2))
plt.plot(xh, yh1, color='b', linewidth=2)
plt.plot(xh, yh2, color='r', linewidth=2)
plt.plot(xh, yh3, color='g', linewidth=2)
plt.plot(xh, yh1 + yh2 + yh3, color='purple', linewidth=3)
# plt.errorbar(xdatap,y,xerr=wdith/2,ls='none', yerr=yerr,color='k',linewidth=2)
# plt.plot(xdatap, ydata,'.',color='k')
plt.ylim(0, np.max(ydata) + 2)
plt.xlabel('Peculiar Velocity (km/s)')
plt.ylabel('N$_{gal}$')
plt.text(-4800, 15, '$\mu_{2}$-$\mu_{1}$ = ' + str(int(m2 - m1)) + ' km/s')
plt.savefig(str(wdith) + "_1sigma_" + str(iters) + "_sig2_" + str(sig2) + "_hist.ps")
divi = -1800
memlow = np.array([[0 for x in range(2)] for y in range(1)])
memhigh = np.array([[0 for x in range(2)] for y in range(1)])
j = 0
k = 0
plt.show()
I have to make a calculator with argv.sys. When I run my code I keep getting this error:
>>> "C:\Users\admin\Desktop\uni\Informatik BW\assignment.py" + rect 0 0 10 10
File "<stdin>", line 1
"C:\Users\admin\Desktop\uni\Informatik BW\assignment.py" + rect 0 0 10 10
^
SyntaxError: invalid syntax
>>>
Here is my program:
import sys
import math
def area_rectangle(x,y,widht,height):
return (widht*height)
def xy_centroid_rectangle(x,y):
return (k + l * 0.5)
#def area_circle(x,y,r):
#return (r*r*math.pi)
#def xy_centroid_circle(k,r):
# return ((4 * r / 3 * math.pi) * 2)
#def area_half_circle(x,y,r):
# return (r * r * math.pi / 2)
#def xy_centroid_half_circle(k,r):
# return (4 * r / 3 * math.pi)
#def area_right_triangle(x,y,a,h):
# return (a * h / 2)
#def xy_centroid_right_triangle(k,l):
# return (a + h + math.sqrt((a * a) + (h * h)))
x = 0
y = 0
a = 0
fx = 0
fy = 0
f = 0
i = 1
while i < len(sys.argv):
vz = sys.argv[i]
print i
print vz
if sys.argv[i + 1] == "rect":
f = area_rectangle(float(sys.argv[i + 2]),float(sys.argv[i + 3]),float(sys.argv[i + 4]),float(sys.argv[i + 5]))
fx = xy_centroid_rectangle(float(sys.argv[i + 2]),float(sys.argv[i + 4]))
fy = xy_centroid_rectangle(float(sys.argv[i + 3]),float(sys.argv[i + 5]))
i += 6
#if sys.argv[i + 1] == "circ":
#f = area_circle(float(sys.argv[i + 2]),float(sys.argv[i + 3]),float(sys.argv[i + 4]))
#fx = xy_centroid_circle(foat(sys.argv[i + 2]),float(sys.argv[i + 4]))
#fy = xy_centroid_circle(foat(sys.argv[i + 3]),float(sys.argv[i + 4]))
#i += 5
#if sys.argv[i + 1] == "halfcirc":
#f = area_circle(float(sys.argv[i + 2]),float(sys.argv[i + 3]),float(sys.argv[i + 4]))
#fx = xy_centroid_circle(foat(sys.argv[i + 2]),float(sys.argv[i + 4]))
#fy = xy_centroid_circle(foat(sys.argv[i + 3]),float(sys.argv[i + 4]))
#i += 5
#if sys.argv[i + 1] == "righttri":
#f = area_rectangle(float(sys.argv[i + 2]),float(sys.argv[i + 3]),float(sys.argv[i + 4]),float(sys.argv[i + 5]))
#fx = xy_centroid_rectangle(float(sys.argv[i + 2]),float(sys.argv[i + 4]))
#fy = xy_centroid_rectangle(float(sys.argv[i + 3]),float(sys.argv[i + 5]))
#i += 6
if vz == "+":
x = (x * a + fx * f) / (a + f)
y = (y * a + fy * f) / (a + f)
a = a + f
if vz == "-":
x = (x * a - fx * f) / (a - f)
y = (y * a - fy * f) / (a - f)
a = a - f
print x
print y
print a
Why am I getting this error?
That's not how you run a python program. Open a CMD (Windows) prompt and write your command line there. You'll probably need to add python in front too.