df['dia_cm'] = df['Rgrid'] * 1e2 * 2 # particle radius in mm
df['time'] = np.ones_like(df.radii_mm)
df['sHeight'] = (heightvec_bound[i_height + 1] +
heightvec_bound[i_height + 1]) / 2
df['mTot_g'] = dataTable['mTot'] * 1e3 # mass in grams
#calculating density
df = mcr.tableOperator.calcRho(df)
df = df[(df['sPhi'] >=
0.015)] #TODO: this kills everything larger than 3.8mm
reducedDataTable = pd.concat([reducedDataTable, df])
reducedDataTable = reducedDataTable[(reducedDataTable['sMult'] > 1.0)]
print(reducedDataTable)
print("?")
#starting the simulation
output = mcr.fullRadar(dicSettings, reducedDataTable)
print(output)
elif PSD_method == "discrete_SP":
#adding required variables
dataTable[
'radii_mm'] = dataTable['dia'] * 1e3 / 2. # particle radius in mm
dataTable['mTot_g'] = dataTable['mTot'] * 1e3 # mass in grams
dataTable['dia_cm'] = dataTable['dia'] * 1e2 # diameter in centimeters
dataTable['sPhi'] = sPhi
dataTable = dataTable[(dataTable['sPhi'] >= 0.015)]
# dataTable['sMult']=1 #(it deactivates the multiplicity)
#calculating density
dataTable = mcr.tableOperator.calcRho(dataTable)
# now generate a table from the McSnow output.
mcTable = mcr.getMcSnowTable(dicSettings['dataPath'])
print('selecting time step = 600 min ')
#-- now select time step to use (600s is usually used)
selTime = 600.
times = mcTable['time']
mcTable = mcTable[times == selTime]
mcTable = mcTable.sort_values('sHeight')
#print(mcTable.sPhi)
print(
'getting things done :) -> calculating radar variables for {0}GHz'.format(
freq))
#-- now the full polarimetric output is generated (KDP, aswell as spec_H and spec_V, from which you can calculate ZeH, ZeV, ZDR, sZDR)
#mcr.fullRadar(dicSettings,mcTable)
#quit()
output = mcr.fullRadar(dicSettings, mcTable)
print(output)
for wl in dicSettings['wl']:
wlStr = '{:.2e}'.format(wl)
if (dicSettings['scatSet']['mode']
== 'SSRGA') or (dicSettings['scatSet']['mode']
== 'Rayleigh') or (dicSettings['scatSet']['mode']
== 'SSRGA-Rayleigh'):
output['Ze_H_{0}'.format(wlStr)] = output['spec_H_{0}'.format(
wlStr)].sum(dim='vel')
output['MDV_H_{0}'.format(
wlStr)] = (output['spec_H_{0}'.format(wlStr)] * output['vel']).sum(
dim='vel') / output['Ze_H_{0}'.format(wlStr)]
else:
output['Ze_H_{0}'.format(wlStr)] = output['spec_H_{0}'.format(