import wafo.plotbackend.plotbackend as plt
import numpy as np

# pyreport -o chapter2.html chapter2.py

#! CHAPTER2 Modelling random loads and stochastic waves
#!=======================================================
#!
#! Chapter2 contains the commands used in Chapter 2 of the tutorial and
#! present some tools for analysis of random functions with
#! respect to their correlation, spectral and distributional properties.
#! The presentation is divided into three examples:
#!
#! Example1 is devoted to estimation of different parameters in the model.
#! Example2 deals with spectral densities and
#! Example3 presents the use of WAFO to simulate samples of a Gaussian
#! process.
#!
#! Some of the commands are edited for fast computation.
#!
#! Section 2.1 Introduction and preliminary analysis
#!====================================================
#! Example 1: Sea data
#!----------------------
#! Observed crossings compared to the expected for Gaussian signals

import wafo
import wafo.objects as wo
xx = wafo.data.sea()
me = xx[:, 1].mean()
sa = xx[:, 1].std()
xx[:, 1] -= me
ts = wo.mat2timeseries(xx)
tp = ts.turning_points()

cc = tp.cycle_pairs()
lc = cc.level_crossings()
lc.plot()
plt.show()

#! Average number of upcrossings per time unit
#!----------------------------------------------
#! Next we compute the mean frequency as the average number of upcrossings
#! per time unit of the mean level (= 0); this may require interpolation in the
#! crossing intensity curve, as follows.
T = xx[:, 0].max() - xx[:, 0].min()
f0 = np.interp(0, lc.args, lc.data, 0) / T  # zero up-crossing frequency
print('f0 = %g' % f0)

#! Turningpoints and irregularity factor
#!----------------------------------------

fm = len(tp.data) / (2 * T)   # frequency of maxima
alfa = f0 / fm                # approx Tm24/Tm02

print('fm = %g, alpha = %g, ' % (fm, alfa))

#! Visually examine data
#!------------------------
#! We finish this section with some remarks about the quality
#! of the measured data. Especially sea surface measurements can be
#! of poor quality. We shall now check the  quality of the dataset {\tt xx}.
#! It is always good practice to visually examine the data
#! before the analysis to get an impression of the quality,
#! non-linearities and narrow-bandedness of the data.
#! First we shall plot the data and zoom in on a specific region.
#! A part of sea data is visualized with the following commands
plt.clf()
ts.plot_wave('k-', tp, '*', nfig=1, nsub=1)

plt.axis([0, 2, -2, 2])
plt.show()

#! Finding possible spurious points
#!------------------------------------
#! However, if the amount of data is too large for visual examinations one
#! could use the following criteria to find possible spurious points. One
#! must be careful using the criteria for extremevalue analysis, because
#! it might remove extreme waves that are OK and not spurious.

import wafo.misc as wm
dt = ts.sampling_period()
# dt = np.diff(xx[:2,0])
dcrit = 5 * dt
ddcrit = 9.81 / 2 * dt * dt
zcrit = 0
inds, indg = wm.findoutliers(ts.data, zcrit, dcrit, ddcrit, verbose=True)

#! Section 2.2 Frequency Modeling of Load Histories
#!----------------------------------------------------
#! Periodogram: Raw spectrum
#!
plt.clf()
Lmax = 9500
S = ts.tospecdata(L=Lmax)
S.plot()
plt.axis([0, 5, 0, 0.7])
plt.show()

#! Calculate moments
#!-------------------
mom, text = S.moment(nr=4)
print('sigma = %g, m0 = %g' % (sa, np.sqrt(mom[0])))

#! Section 2.2.1 Random functions in Spectral Domain - Gaussian processes
#!--------------------------------------------------------------------------
#! Smoothing of spectral estimate
#!----------------------------------
#! By decreasing Lmax the spectrum estimate becomes smoother.

plt.clf()
Lmax0 = 200
Lmax1 = 50
S1 = ts.tospecdata(L=Lmax0)
S2 = ts.tospecdata(L=Lmax1)
S1.plot('-.')
S2.plot()
plt.show()

#! Estimated autocovariance
#!----------------------------
#! Obviously knowing the spectrum one can compute the covariance
#! function. The following code will compute the covariance for the
#! unimodal spectral density S1 and compare it with estimated
#! covariance of the signal xx.
plt.clf()
Lmax = 85
R1 = S1.tocovdata(nr=1)
Rest = ts.tocovdata(lag=Lmax)
R1.plot('.')
Rest.plot()
plt.axis([0, 25, -0.1, 0.25])
plt.show()

#! We can see in Figure below that the covariance function corresponding to
#! the spectral density S2 significantly differs from the one estimated
#! directly from data.
#! It can be seen in Figure above that the covariance corresponding to S1
#! agrees much better with the estimated covariance function

plt.clf()
R2 = S2.tocovdata(nr=1)
R2.plot('.')
Rest.plot()
plt.show()

#! Section 2.2.2 Transformed Gaussian models
#!-------------------------------------------
#! We begin with computing skewness and kurtosis
#! for the data set xx and compare it with the second order wave approximation
#! proposed by Winterstein:
import wafo.stats as ws
rho3 = ws.skew(xx[:, 1])
rho4 = ws.kurtosis(xx[:, 1])

sk, ku = S1.stats_nl(moments='sk')

#! Comparisons of 3 transformations
plt.clf()
import wafo.transform.models as wtm
gh = wtm.TrHermite(mean=me, sigma=sa, skew=sk, kurt=ku).trdata()
g = wtm.TrLinear(mean=me, sigma=sa).trdata()  # Linear transformation
glc, gemp = lc.trdata(mean=me, sigma=sa)

glc.plot('b-')  # Transf. estimated from level-crossings
gh.plot('b-.')  # Hermite Transf. estimated from moments
g.plot('r')
plt.grid('on')
plt.show()

#! Test Gaussianity of a stochastic process
#!------------------------------------------
#! TESTGAUSSIAN simulates  e(g(u)-u) = int (g(u)-u)^2 du  for Gaussian processes
#! given the spectral density, S. The result is plotted if test0 is given.
#! This is useful for testing if the process X(t) is Gaussian.
#! If 95% of TEST1 is less than TEST0 then X(t) is not Gaussian at a 5% level.
#!
#! As we see from the figure below: none of the simulated values of test1 is
#! above 1.00. Thus the data significantly departs from a Gaussian distribution.
plt.clf()
test0 = glc.dist2gauss()
#! the following test takes time
N = len(xx)
test1 = S1.testgaussian(ns=N, cases=50, test0=test0)
is_gaussian = sum(test1 > test0) > 5
print(is_gaussian)
plt.show()

#! Normalplot of data xx
#!------------------------
#! indicates that the underlying distribution has a "heavy" upper tail and a
#! "light" lower tail.
plt.clf()
import pylab
ws.probplot(ts.data.ravel(), dist='norm', plot=pylab)
plt.show()
#! Section 2.2.3 Spectral densities of sea data
#!-----------------------------------------------
#! Example 2: Different forms of spectra
#!
import wafo.spectrum.models as wsm
plt.clf()
Hm0 = 7
Tp = 11
spec = wsm.Jonswap(Hm0=Hm0, Tp=Tp).tospecdata()
spec.plot()
plt.show()

#! Directional spectrum and Encountered directional spectrum
#! Directional spectrum
plt.clf()
D = wsm.Spreading('cos2s')
Sd = D.tospecdata2d(spec)
Sd.plot()
plt.show()


##!Encountered directional spectrum
##!---------------------------------
#clf()
#Se = spec2spec(Sd,'encdir',0,10);
#plotspec(Se), hold on
#plotspec(Sd,1,'--'), hold off
##!wafostamp('','(ER)')
#disp('Block = 17'),pause(pstate)
#
##!#! Frequency spectra
#clf
#Sd1 =spec2spec(Sd,'freq');
#Sd2 = spec2spec(Se,'enc');
#plotspec(spec), hold on
#plotspec(Sd1,1,'.'),
#plotspec(Sd2),
##!wafostamp('','(ER)')
#hold off
#disp('Block = 18'),pause(pstate)
#
##!#! Wave number spectrum
#clf
#Sk = spec2spec(spec,'k1d')
#Skd = spec2spec(Sd,'k1d')
#plotspec(Sk), hold on
#plotspec(Skd,1,'--'), hold off
##!wafostamp('','(ER)')
#disp('Block = 19'),pause(pstate)
#
##!#! Effect of waterdepth on spectrum
#clf
#plotspec(spec,1,'--'), hold on
#S20 = spec;
#S20.S = S20.S.*phi1(S20.w,20);
#S20.h = 20;
#plotspec(S20),  hold off
##!wafostamp('','(ER)')
#disp('Block = 20'),pause(pstate)
#
##!#! Section 2.3 Simulation of transformed Gaussian process
##!#! Example 3: Simulation of random sea
##! The reconstruct function replaces the spurious points of seasurface by
##! simulated data on the basis of the remaining data and a transformed Gaussian
##! process. As noted previously one must be careful using the criteria
##! for finding spurious points when reconstructing a dataset, because
##! these criteria might remove the highest and steepest waves as we can see
##! in this plot where the spurious points is indicated with a '+' sign:
##!
#clf
#[y, grec] = reconstruct(xx,inds);
#waveplot(y,'-',xx(inds,:),'+',1,1)
#axis([0 inf -inf inf])
##!wafostamp('','(ER)')
#disp('Block = 21'),pause(pstate)
#
##! Compare transformation (grec) from reconstructed (y)
##! with original (glc) from (xx)
#clf
#trplot(g), hold on
#plot(gemp(:,1),gemp(:,2))
#plot(glc(:,1),glc(:,2),'-.')
#plot(grec(:,1),grec(:,2)), hold off
#disp('Block = 22'),pause(pstate)
#
##!#!
#clf
#L = 200;
#x = dat2gaus(y,grec);
#Sx = dat2spec(x,L);
#disp('Block = 23'),pause(pstate)
#
##!#!
#clf
#dt = spec2dt(Sx)
#Ny = fix(2*60/dt) #! = 2 minutes
#Sx.tr = grec;
#ysim = spec2sdat(Sx,Ny);
#waveplot(ysim,'-')
##!wafostamp('','(CR)')
#disp('Block = 24'),pause(pstate)
#
#! Estimated spectrum compared to Torsethaugen spectrum
#!-------------------------------------------------------

plt.clf()
fp = 1.1
dw = 0.01
H0 = S1.characteristic('Hm0')[0]
St = wsm.Torsethaugen(Hm0=H0,Tp=2*np.pi/fp).tospecdata(np.arange(0,5+dw/2,dw))
S1.plot()
St.plot('-.')
plt.axis([0, 6, 0, 0.4])
plt.show()


#! Transformed Gaussian model compared to Gaussian model
#!--------------------------------------------------------
dt = St.sampling_period()
va, sk, ku = St.stats_nl(moments='vsk')
#sa = sqrt(va)
gh = wtm.TrHermite(mean=me, sigma=sa, skew=sk, kurt=ku, ysigma=sa)

ysim_t = St.sim(ns=240, dt=0.5)
xsim_t = ysim_t.copy()
xsim_t[:,1] = gh.gauss2dat(ysim_t[:,1])

ts_y = wo.mat2timeseries(ysim_t)
ts_x = wo.mat2timeseries(xsim_t)
ts_y.plot_wave(sym1='r.', ts=ts_x, sym2='b', sigma=sa, nsub=5, nfig=1)
plt.show()
