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Python numpy.str函数代码示例

本文整理汇总了Python中numpy.str函数的典型用法代码示例。如果您正苦于以下问题:Python str函数的具体用法?Python str怎么用?Python str使用的例子?那么恭喜您, 这里精选的函数代码示例或许可以为您提供帮助。


在下文中一共展示了str函数的15个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。

示例1: roms_to_swan_bathy_curv

def roms_to_swan_bathy_curv(hisfile,outfld):
  ''' 
  Generate a SWAN bathymetry file from either a ROMS history or bathymetry input
  file. 
  
  roms_to_swan_bathy_curv(hisfile,outfld)
  
  Parameters
  ----------
  hisfile  : ROMS history or bathymetry input netCDF file
  outfld   : Folder to save the output files
  
  Returns
  -------
  Two text files (swan_bathy.bot, swan_coord.grd) that contain the bathymetry 
  and coordinates of the grid for SWAN input. 
  
  Notes
  -----
    
    
  '''  
   
  # Load variables of interest from the ocean_his.nc file
  ncfile = netCDF4.Dataset(hisfile,'r')  
  h = ncfile.variables['h'][:]
  x_rho = ncfile.variables['x_rho'][:]
  y_rho = ncfile.variables['y_rho'][:]  
  ncfile.close()
  
   
  # Print text file with extended and interpolated bathymetry
  fid = open(outfld+'/swan_bathy.bot', 'w')  
  for aa in range(h.shape[0]):
      for bb in range(h.shape[1]):
          fid.write('%12.4f' % h[aa,bb])
      fid.write('\n')
  fid.close()
  
  # Print text file with extended and interpolated bathymetry
  fid = open(outfld+'/swan_coord.bot', 'w')  
  for aa in range(x_rho.shape[0]):
      for bb in range(x_rho.shape[1]):
          fid.write('%12.6f' % x_rho[aa,bb])
          fid.write('\n')
  for aa in range(y_rho.shape[0]):
      for bb in range(y_rho.shape[1]):
          fid.write('%12.6f' % y_rho[aa,bb])
          fid.write('\n')          
  fid.close()  
  
  #---------------------------------------------------------- Output for swan.in
  print ' '
  print "========================================================"
  print "Created swan_coord.grd and swan_bathy.bot"
  print ('CGRID CURVILINEAR ' + np.str(h.shape[1]-1) + ' ' + 
         np.str(h.shape[0]-1) + ' CIRCLE ...')
  print ('INPGRID BOTTTOM CURVILINEAR 0 0 ' + np.str(h.shape[1]-1) + ' ' + 
         np.str(h.shape[0]-1) + ' EXC ...')
  print "========================================================"  
开发者ID:vilandra,项目名称:pynmd,代码行数:60,代码来源:roms_post.py

示例2: update_task

 def update_task(self, filename):
     #set scheduled
     with open(filename) as f:
         d = dict(filter(None, csv.reader(f,  delimiter=' ', skipinitialspace=True))) 
         taskid = d['taskID']
         AST= d['AST']                 
         f.close()
 
     #update task status in emoncms
     h = httplib2.Http("/tmp/emoncms/.cache")
     minutes=np.int(AST)%3600
     minutes=minutes/60
     hours=np.int(AST)/3600 
          
     request = "{'status':1,'AST':'"+np.str(hours)+":"+np.str(minutes)+"'}"
     h.request("http://localhost/emoncms/mas/update.json?id="+taskid+"&json="+request+"&apikey="+self.apikey, "GET")
     sys.stderr.write("http://localhost/emoncms/mas/update.json?id="+taskid+"&json="+request+"&apikey="+self.apikey)
     #delay should be not 20 but AST-Time.time
     now = datetime.datetime.now()
     midnight = now.replace(hour=0, minute=0, second=0, microsecond=0)
     seconds = (now - midnight).seconds
     countdown = np.int(AST)-seconds
     #countdown =20
     if(countdown > 0):
         t=Timer(countdown, self.taskexec, [taskid])
         t.start()
         self.scheduled[taskid]=0
开发者ID:BentHeier,项目名称:IT2901-emoncms,代码行数:27,代码来源:schedulerd.py

示例3: read_input_spectra

def read_input_spectra(fname, numbvals):
    # Read grid of model spectra from the <fname> file
    #
    # :rtype: list of tuples containing model spectra.
    #
    # :param fname: name of the file containing the grid of model spectra.
    # :param numbvals: list with total grid number of model parameters.

    d = np.loadtxt(fname)
    parameter_combinations = np.prod(numbvals)
    numspectra = len(d.T) - 1
    # spectra in columns, 1st column is energy grid, skip it
    if numspectra != parameter_combinations:
        raise NameError(
            fname
            + ": No. of spectra "
            + np.str(numspectra)
            + ", different from declared param combinations "
            + np.str(parameter_combinations)
            + "\n"
        )
    input_spectra = []
    for i in range(len(d.T) - 1):
        # d[:-1] - match no. of energy bins;
        # T[1:] - skip the 1st column with energy vector
        input_spectra.append(tuple(d[:-1].T[1:][i]))

    return input_spectra
开发者ID:malgosias,项目名称:2015-12-16-code-sample-3,代码行数:28,代码来源:tabmod.py

示例4: load_fortranfile

def load_fortranfile(T):

	if T < 100:
		file1 = '../outputs/psi1/psi1_0'+np.str(T)+'.bin'
		file2 = '../outputs/psi2/psi2_0'+np.str(T)+'.bin'

	else:
		file1 = '../outputs/psi1/psi1_'+np.str(T)+'.bin'
		file2 = '../outputs/psi2/psi2_'+np.str(T)+'.bin'		


	PSI1 = fortranfiles.FortranFile(file1) 
	PSI1 = PSI1.readReals()


	PSI2 = fortranfiles.FortranFile(file2) 
	PSI2 = PSI2.readReals()



	# Redimensionalizing files
	PSI1 = PSI1.reshape((257,512))
	PSI2 = PSI2.reshape((257,512))



	return PSI1,PSI2
开发者ID:tiagobilo,项目名称:tiagobilo.github.io,代码行数:27,代码来源:philips_model_project.py

示例5: main

def main():
    if len(sys.argv) < 4:
        print_usage("Not enough arguments!")
    alpha = numpy.float64(sys.argv[1])
    filename= numpy.str(sys.argv[2])
    k_limit = 12
    species = []
    for i, s in enumerate(sys.argv[3:]):
        species.append(numpy.str(s))
    species.sort()
    print("species",str(species))
    print("Reading %s" % filename)
    data = atpy_csv(filename)

    if species == 'Overall' or species == 'overall':
        data = filter_by_keyvalue(data, 'alpha', alpha)

    metrs = []
    for s in species:
        print("Calculating %s at %s" % ('mean', s))
        metrs.append(calc_metrics(data, k_limit, alpha, s))
        print(metrs[-1])

    all_metrics = dict(zip(species, metrs))

    metr_fname = "./figures/%s-ALL-metrics-%d-%s.pdf" % (str(species).replace(']','').replace('[','').replace("'",""), k_limit, str(numpy.around(alpha, decimals=2)))
    plot_metrics_per_k(species, alpha, all_metrics, 'Algorithm: ' + filename.split('.')[0], metr_fname)

    pvr_fname = "./figures/%s-ALL-pvr-%d-%s.pdf" % (str(species).replace(']','').replace('[','').replace("'",""), k_limit, str(numpy.around(alpha, decimals=2)))
    print(pvr_fname)
    plot_precision_v_recall(species, alpha, all_metrics, 'Algorithm: ' + filename.split('.')[0], pvr_fname)

    return 0
开发者ID:jmcgover,项目名称:cplop,代码行数:33,代码来源:species.py

示例6: calc_test_press

    def calc_test_press(self, path_const='T'):

        TOL = 1e-3

        Nsamp = 10001
        eos_mod = self.load_eos(path_const=path_const)

        V0, = eos_mod.get_param_values(param_names='V0')
        V0 += -.137
        eos_mod.set_param_values(V0,param_names='V0')

        V0get, = eos_mod.get_param_values(param_names='V0')

        assert V0 == V0get, 'Must be able to store and retrieve non-integer values'

        assert np.abs(eos_mod.press(V0))<TOL/100,(
            'pressure at V0 must be zero by definition'
        )

        Vmod_a = np.linspace(.7,1.2,Nsamp)*V0
        dV = Vmod_a[1] - Vmod_a[0]

        press_a = eos_mod.press(Vmod_a)
        energy_a = eos_mod.energy(Vmod_a)

        abs_err, rel_err, range_err = self.numerical_deriv(
            Vmod_a, energy_a, press_a, scale=-core.CONSTS['PV_ratio'])

        assert range_err < TOL, 'range error in Press, ' + np.str(range_err) + \
            ', must be less than TOL, ' + np.str(TOL)
开发者ID:aswolf,项目名称:xmeos,代码行数:30,代码来源:test_models_compress.py

示例7: test_press_simple

    def test_press_simple(self, kind_compress='Vinet',
                          compress_path_const='T',
                          kind_gamma='GammaFiniteStrain',
                          kind_RTpoly='V', RTpoly_order=5, natom=1,
                          kind_electronic='CvPowLaw', apply_electronic=True):

        TOL = 1e-3
        Nsamp = 10001
        eos_mod = self.load_eos(kind_compress=kind_compress,
                                compress_path_const=compress_path_const,
                                kind_gamma=kind_gamma, kind_RTpoly=kind_RTpoly,
                                RTpoly_order=RTpoly_order, natom=natom,
                                kind_electronic=kind_electronic,
                                apply_electronic=apply_electronic)

        refstate_calc = eos_mod.calculators['refstate']
        T0 = refstate_calc.ref_temp()
        V0 = refstate_calc.ref_volume()
        S0 = refstate_calc.ref_entropy()
        # V0, T0, S0 = eos_mod.get_param_values(param_names=['V0','T0','S0'])

        Vmod_a = np.linspace(.7,1.2,Nsamp)*V0
        T = 8000
        dV = Vmod_a[1] - Vmod_a[0]

        P_a = eos_mod.press(Vmod_a, T)
        F_a = eos_mod.helmholtz_energy(Vmod_a, T)
        abs_err, rel_err, range_err = self.numerical_deriv(
              Vmod_a, F_a, P_a, scale=-core.CONSTS['PV_ratio'])

        S_a = eos_mod.entropy(Vmod_a, T)


        assert abs_err < TOL, ('abs error in Press, ' + np.str(abs_err) +
                                 ', must be less than TOL, ' + np.str(TOL))
开发者ID:aswolf,项目名称:xmeos,代码行数:35,代码来源:test_models_composite.py

示例8: freq_spec_1d

def freq_spec_1d(eta,dt=1,verbose=True):
    """
    Computes the frequency spectrum from a given time series.
    
    freq,spec = freq_spec_1d(eta,dt,verbose)
    
    PARAMETERS:
    -----------
    eta      : Time series of water surface elevation [m]
    dt       : Time step [s]
    verbose  : Display computed bulk parameters to the screen
    
    RETURNS:
    --------
    freq     : Frequency vector
    spec     : Variance spectrum (Power spectrum)
    
    NOTES:
    ------
    This is really a copy of gsignal.psdraw. If results differ, trust gsignal
      this code will not be updated.
    """
    
    # Remove mean
    eta -= eta.mean()

    # Compute record length
    N = eta.shape[0]
    
    # Compute fourier frequencies
    fj = np.fft.fftfreq(N,dt)

    # Compute power spectral density (Cooley-Tukey Method)
    yf = np.fft.fft(eta)/N
    psd = N*dt*yf*np.conjugate(yf)

    # One sided psd from dft
    if np.mod(N,2) == 0:
        sf = np.concatenate((np.array([psd[0]]),2.0*psd[1:N/2],
                             np.array([psd[N/2]])))
        freq_amp = np.abs(np.concatenate((np.array([fj[0]]),fj[1:N/2],
                                          np.array([fj[N/2]]))))
    else:
        sf = np.concatenate((np.array([psd[0]]),2.0*psd[1:(N+1)/2]))
        freq_amp = np.abs(np.concatenate((np.array([fj[0]]),fj[1:(N+1)/2])))

    sf = sf.real
    
    if verbose:
        print("===============================================")
        print("Bulk Wave Parameters:")
        print("Hs = " + np.str(4.004*np.sqrt(np.trapz(sf,freq_amp))) + "m")
        print("H1 = "+np.str(4.004*np.sqrt(np.trapz(sf,freq_amp))*2.0/3.0)+"m")
        print("Spectral Parameters:")
        print("Nyquist Frequency = " + np.str(1.0/(2.0*dt)) + "Hz")
        print("Frequency interval = " + np.str(1.0/(N*dt)) + "Hz")
        print("===============================================")

    # End of function
    return freq_amp,sf
开发者ID:vilandra,项目名称:pynmd,代码行数:60,代码来源:funwave_post.py

示例9: _calc_test_heat_capacity

    def _calc_test_heat_capacity(self, kind_compress='Vinet',
                                 compress_path_const='T',
                                 kind_gamma='GammaFiniteStrain',
                                 kind_RTpoly='V', RTpoly_order=5, natom=1,
                                 kind_electronic='None',
                                 apply_electronic=False):

        TOL = 1e-3
        Nsamp = 10001

        eos_mod = self.load_eos(kind_compress=kind_compress,
                                compress_path_const=compress_path_const,
                                kind_gamma=kind_gamma, kind_RTpoly=kind_RTpoly,
                                RTpoly_order=RTpoly_order, natom=natom,
                                kind_electronic=kind_electronic,
                                apply_electronic=apply_electronic)

        Tmod_a = np.linspace(3000.0, 8000.0, Nsamp)

        V0, = eos_mod.get_param_values(param_names=['V0'])
        # Vmod = V0*(0.6+.5*np.random.rand(Nsamp))
        Vmod = V0*0.7

        thermal_energy_a = eos_mod.thermal_energy(Vmod, Tmod_a)
        heat_capacity_a = eos_mod.heat_capacity(Vmod, Tmod_a)

        abs_err, rel_err, range_err = self.numerical_deriv(
            Tmod_a, thermal_energy_a, heat_capacity_a, scale=1)

        Cvlimfac = eos_mod.calculators['thermal']._get_Cv_limit()
        assert rel_err < TOL, 'rel-error in Cv, ' + np.str(rel_err) + \
            ', must be less than TOL, ' + np.str(TOL)
开发者ID:aswolf,项目名称:xmeos,代码行数:32,代码来源:test_models_composite.py

示例10: calc_test_RTcoefs

    def calc_test_RTcoefs(self, kind_compress='Vinet',
                           compress_path_const='T',
                           kind_gamma='GammaFiniteStrain', kind_RTpoly='V',
                           RTpoly_order=5, natom=1, kind_electronic='None',
                           apply_electronic=False):

        TOL = 1e-3

        Nsamp = 10001
        eos_mod = self.load_eos(kind_compress=kind_compress,
                                compress_path_const=compress_path_const,
                                kind_gamma=kind_gamma, kind_RTpoly=kind_RTpoly,
                                RTpoly_order=RTpoly_order, natom=natom,
                                kind_electronic=kind_electronic,
                                apply_electronic=apply_electronic)

        V0, = eos_mod.get_param_values(param_names='V0')
        Vmod_a = np.linspace(.5,1.2,Nsamp)*V0
        dV = Vmod_a[1] - Vmod_a[0]

        bcoef_a = eos_mod.calc_RTcoefs(Vmod_a)
        bcoef_deriv_a = eos_mod.calc_RTcoefs_deriv(Vmod_a)

        b_abs_err, b_rel_err, b_range_err = self.numerical_deriv(
            Vmod_a, bcoef_a, bcoef_deriv_a, scale=1)

        assert b_range_err < TOL, 'range error in bcoef, ' + \
            np.str(b_range_err) + ', must be less than TOL, ' + np.str(TOL)
开发者ID:aswolf,项目名称:xmeos,代码行数:28,代码来源:test_models_composite.py

示例11: test_RTcoefs

    def test_RTcoefs(self, kind_compress='Vinet', compress_order=3,
                     compress_path_const='T', kind_RTpoly='V',
                     RTpoly_order=5, natom=1):

        TOL = 1e-3

        Nsamp = 10001
        eos_mod = self.load_eos(kind_compress=kind_compress,
                                compress_order=compress_order,
                                compress_path_const=compress_path_const,
                                kind_RTpoly=kind_RTpoly,
                                RTpoly_order=RTpoly_order,
                                natom=natom)

        V0, = eos_mod.get_param_values(param_names='V0')
        Vmod_a = np.linspace(.5,1.2,Nsamp)*V0
        dV = Vmod_a[1] - Vmod_a[0]

        acoef_a, bcoef_a = eos_mod.calc_RTcoefs(Vmod_a)
        acoef_deriv_a, bcoef_deriv_a = eos_mod.calc_RTcoefs_deriv(Vmod_a)

        a_abs_err, a_rel_err, a_range_err = self.numerical_deriv(
            Vmod_a, acoef_a, acoef_deriv_a, scale=1)

        b_abs_err, b_rel_err, b_range_err = self.numerical_deriv(
            Vmod_a, bcoef_a, bcoef_deriv_a, scale=1)


        assert a_range_err < TOL, 'range error in acoef, ' + \
            np.str(a_range_err) + ', must be less than TOL, ' + np.str(TOL)

        assert b_range_err < TOL, 'range error in bcoef, ' + \
            np.str(b_range_err) + ', must be less than TOL, ' + np.str(TOL)
开发者ID:aswolf,项目名称:xmeos,代码行数:33,代码来源:test_models_composite.py

示例12: laserScan2D

def laserScan2D(width, height, delta, peakArea, fileName):
    # Scans an area with given width and height at a
    # step rate of delta. peakArea is int value for
    # the location of peak with a scale from 0 to 10,000

    startTime = time.clock()
    h = 0
    w = 0
    n = 0
    m = 0

    x = np.arange(0, width + delta, delta)
    y = np.arange(0, height + delta, delta)
    Y, X = np.meshgrid(y, x)
    tValues = np.zeros((np.size(x), np.size(y)))
    vValues = np.zeros((np.size(x), np.size(y)))

    # set up scope
    scanRange = 1000
    scope = vi.instrument("TCPIP::138.67.12.235::INSTR")
    sRead.setParam(scope, peakArea - scanRange, peakArea + scanRange)

    # get motor and zero location
    motor = mC.setupMotor()

    while w <= width:
        h = 0
        m = 0
        while h <= height:
            mC.moveTo(motor, w, h)
            time.sleep(0.5)
            x, y = sRead.getData(scope, peakArea - scanRange, peakArea + scanRange)
            t, v = findPeak(x, y)
            tValues[n, m] = t
            vValues[n, m] = v
            h = h + delta
            m = m + 1
        w = w + delta
        n = n + 1

        # Estimates Time Left
        timeLeft = (width - w) / w * (time.clock() - startTime) / 60
        print "Est. Time Left " + np.str(timeLeft) + "min"
    mC.moveTo(motor, 0, 0)

    # Contour Plot of Time
    makePlot2D(X, Y, tValues, fileName + " Time")

    # Contour Plot of Voltage
    makePlot2D(X, Y, vValues, fileName + " Voltage")

    # File Output
    np.savez(fileName + ".npz", X=X, Y=Y, tValues=tValues, vValues=vValues)

    # Time Taken Calc
    timeTaken = (time.clock() - startTime) / 60  # in min
    print "Time Taken " + np.str(timeTaken)
    motor.close()
    scope.close()
    return timeTaken, tValues
开发者ID:ngreeney,项目名称:Infrared-Laser-Scan,代码行数:60,代码来源:laserScan8.py

示例13: wave_length

def wave_length(period, h, verbose=True):
    """
    Compute wave length using linear wave theory

    Parameters
    ----------
    period   : wave period [s]
    h        : water depth [m]

    Results
    -------
    wl_int   : real wave length [m]

    Screen output
    -------------
    wl_deep  : deep water wave length [m]
    wl_sha   : shallow water wave length [m]

    """

    wl_deep = 9.81 * period ** 2 / 2.0 / np.pi
    wl_sha = period * np.sqrt(9.81 * h)
    k = dispersion(period, h)
    wl_int = 9.81 / 2.0 / np.pi * period ** 2 * np.tanh(k * h)

    if verbose:
        print(" ")
        print("---------------------------------------------------------")
        print("Wave Length deep water approx      = " + np.str(wl_deep) + " m")
        print("Wave Length shallow water approx   = " + np.str(wl_sha) + " m")
        print("Wave Length linear wave theory     = " + np.str(wl_int) + " m")
        print("---------------------------------------------------------")
        print(" ")

    return wl_int
开发者ID:garciaga,项目名称:pynmd,代码行数:35,代码来源:waves.py

示例14: wave_length

def wave_length(period,h):
    '''
    Compute wave length using linear wave theory
    
    Parameters
    ----------
    period   : wave period [s]
    h        : water depth [m]
    
    Results
    -------
    wl_int   : real wave length [m]
    
    Screen output
    -------------
    wl_deep  : deep water wave length [m]
    wl_sha   : shallow water wave length [m]
    
    '''
    
    wl_deep = 9.81 * period**2 / 2.0 / np.pi
    wl_sha = period * np.sqrt(9.81 * h)
    k = dispersion(period,h)
    wl_int = 9.81 / 2.0 / np.pi * period**2 * np.tanh(k*h)
    
    print(' ')
    print('---------------------------------------------------------')
    print('Wave Length deep water approx      = ' + np.str(wl_deep) + ' m')
    print('Wave Length shallow water approx   = ' + np.str(wl_sha) + ' m')
    print('Wave Length linear wave theory     = ' + np.str(wl_int) + ' m')
    print('---------------------------------------------------------')
    print(' ')
    
    return wl_int
开发者ID:vilandra,项目名称:pynmd,代码行数:34,代码来源:waves.py

示例15: save_orbit

def save_orbit( x, y, z, filename ):
	ff = open( filename + '.3d', 'w' )
	for i in range(len(x)):
		ff.write( np.str(x[i]) + "," +
				  np.str(y[i]) + "," +
				  np.str(z[i]) + "\n" )
	ff.close()
	return
开发者ID:HacktheUniverse,项目名称:twitterverse,代码行数:8,代码来源:plot_orbits.py


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