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Calculates observed bulk density #59

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2 changes: 2 additions & 0 deletions .gitignore
Original file line number Diff line number Diff line change
Expand Up @@ -34,4 +34,6 @@ build/
fwl_data*/
dist/
.pytest_cache
.ruff_cache


28 changes: 17 additions & 11 deletions README.md
Original file line number Diff line number Diff line change
Expand Up @@ -3,21 +3,27 @@

## JANUS (1D convective atmosphere model)

Generates a temperature profile using the generalised moist pseudoadiabat and a prescribed stratosphere. Calculates radiative fluxes using SOCRATES.
Generates a temperature profile using the generalised moist pseudoadiabat and a prescribed stratosphere. Calculates radiative fluxes using SOCRATES.

Pronounced *jan-us*. *Jan* as in "january", and *us* as in the collective pronoun.

### Documentation
https://proteus-code.readthedocs.io

### Contributors (abbreviations & email addresses):
* TL - Tim Lichtenberg ([email protected])
* MH - Mark Hammond ([email protected])
* RB – Ryan Boukrouche ([email protected])
* RJG – RJ Graham ([email protected])
* HN - Harrison Nicholls ([email protected])
* HII - Hamish Innes ([email protected])
* LS - Laurent Soucasse ([email protected])
https://fwl-proteus.readthedocs.io

## Contributors

| Name | Email address |
| - | - |
Tim Lichtenberg | tim.lichtenberg[at]rug.nl |
Harrison Nicholls | harrison.nicholls[at]physics.ox.ac.uk |
Laurent Soucasse | l.soucasse[at]esciencecenter.nl |
Stef Smeets | s.smeets[at]esciencecenter.nl |
Mark Hammond | mark.hammond[at]physics.ox.ac.uk |
RJ Graham | arejaygraham[at]uchicago.edu |
Raymond Pierrehumbert | raymond.pierrehumbert[at]physics.ox.ac.uk |
Ryan Boukrouche | ryan.boukrouche[at]astro.su.se |
Hamish Innes | hamish.innes[at]fu-berlin.de |


### Repository structure
* `README.md` - This file
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16 changes: 8 additions & 8 deletions src/janus/utils/atmosphere_column.py
Original file line number Diff line number Diff line change
Expand Up @@ -5,7 +5,7 @@
import numpy as np
import netCDF4 as nc
from janus.utils import phys
from janus.utils.height import AtmosphericHeight
from janus.utils.height import integrate_heights
import os, copy, platform, shutil
import pwd
from datetime import datetime
Expand Down Expand Up @@ -172,7 +172,7 @@ def __init__(self, T_surf: float, P_surf: float, P_top: float, pl_radius: float,
self.rho = np.zeros(self.nlev) # Density of atmosphere at a given level
self.ifatm = np.zeros(self.nlev) # Defines nth level to which atmosphere is calculated
self.cp = np.zeros(self.nlev) # Mean heat capacity
self.height_error = True # error when doing hydrostatic integration?
self.height_error = False # error when doing hydrostatic integration?

# Define T and P arrays from surface up
self.tmp[0] = self.ts # K
Expand Down Expand Up @@ -389,12 +389,7 @@ def write_ncdf(self, fpath:str):

# ----------------------
# Calculate gravity and height (in case it hasn't been done already)
self.z = AtmosphericHeight(self, self.planet_mass, self.planet_radius)

self.zl = np.zeros(len(self.z)+1)
for i in range(1,len(self.z)):
self.zl[i] = 0.5 * (self.z[i-1] + self.z[i])
self.zl[0] = 2*self.z[0] - self.zl[1] # estimate TOA height
self.z, self.zl, self.height_error = integrate_heights(self, self.planet_mass, self.planet_radius)

# ----------------------
# Prepare NetCDF
Expand Down Expand Up @@ -454,6 +449,7 @@ def write_ncdf(self, fpath:str):
var_albsurf = ds.createVariable("surf_albedo", 'f4'); # Surface albedo
var_sknd = ds.createVariable("cond_skin_d" ,'f4'); var_sknd.units = "m" # Conductive skin thickness
var_sknk = ds.createVariable("cond_skin_k" ,'f4'); var_sknk.units = "W m-1 K-1" # Conductive skin thermal conductivity
var_zok = ds.createVariable("height_ok" ,'S1'); # Hydrostatic integration is ok

# Store data
var_tstar.assignValue(self.ts)
Expand All @@ -471,6 +467,10 @@ def write_ncdf(self, fpath:str):
var_albsurf.assignValue(self.albedo_s)
var_sknd.assignValue(self.skin_d)
var_sknk.assignValue(self.skin_k)
if self.height_error:
var_zok[0] = 'n'
else:
var_zok[0] = 'y'


# ----------------------
Expand Down
42 changes: 24 additions & 18 deletions src/janus/utils/height.py
Original file line number Diff line number Diff line change
@@ -1,17 +1,17 @@
import numpy as np
import janus.utils.phys as phys

import logging
import logging
log = logging.getLogger("fwl."+__name__)


def gravity( m, r ):
g = phys.G*m/r**2
return g

def AtmosphericHeight(atm, m_planet, r_planet):
def integrate_heights(atm, m_planet, r_planet):

z_profile = np.zeros(len(atm.p))
z = np.zeros(len(atm.p))
grav_s = gravity( m_planet, r_planet )

# Reverse arrays to go from high to low pressure
Expand All @@ -20,39 +20,45 @@ def AtmosphericHeight(atm, m_planet, r_planet):
for vol in atm.vol_list.keys():
atm.x_gas[vol] = atm.x_gas[vol][::-1]

atm.height_error = False
for n in range(0, len(z_profile)-1):
height_error = False
for n in range(0, len(z)-1):

# Gravity with height
grav_z = grav_s * ((r_planet)**2) / ((r_planet + z_profile[n])**2)
grav_z = grav_s * ((r_planet)**2) / ((r_planet + z[n])**2)

# Mean molar mass depending on mixing ratio
mean_molar_mass = 0
for vol in atm.vol_list.keys():
mean_molar_mass += phys.molar_mass[vol]*atm.x_gas[vol][n]

# Use hydrostatic equation to get height difference
dz = phys.R_gas * atm.tmp[n] / (mean_molar_mass * grav_z * atm.p[n]) * (atm.p[n] - atm.p[n+1])
dz = phys.R_gas * atm.tmp[n] / (mean_molar_mass * grav_z * atm.p[n]) * (atm.p[n] - atm.p[n+1])

# Next height
z_profile[n+1] = z_profile[n] + dz
z[n+1] = z[n] + dz

# Check if heights are very large.
# This implies that the hydrostatic/gravity integration failed.
if z_profile[n+1] > 1.0e8:
atm.height_error = True
log.warning("Hydrostatic integration blew up. Setting dummy values for height")
if (z[n+1] > 1.0e8) or (dz > 1e8):
height_error = True
log.error("Hydrostatic integration blew up. Setting dummy values for height")
break

# Set dummy values
if atm.height_error:
z_profile = np.linspace(0.0, 1000.0, len(atm.p))
# Set dummy values
if height_error:
z = np.linspace(0.0, 1000.0, len(atm.p))

# Reverse arrays again back to normal
atm.p = atm.p[::-1]
atm.tmp = atm.tmp[::-1]
for vol in atm.vol_list.keys():
atm.x_gas[vol] = atm.x_gas[vol][::-1]
z_profile = z_profile[::-1]
z = z[::-1]

# Set cell edge values
zl = np.zeros(len(z)+1)
for i in range(1,len(z)):
zl[i] = 0.5 * (z[i-1] + z[i])
zl[0] = 2*z[0] - zl[1] # estimate TOA height

return z_profile
return z, zl, height_error
40 changes: 40 additions & 0 deletions src/janus/utils/observed_rho.py
Original file line number Diff line number Diff line change
@@ -0,0 +1,40 @@
import numpy as np

def calc_observed_rho(atm):
"""Calculate the observed bulk density.

Copied from AGNI.

Parameters
----------
atm : atmos
Atmosphere object from atmosphere_column.py

Returns
----------
rho : float
Observed bulk density [kg m-3]
"""

# transspec_r::Float64 # planet radius probed in transmission [m]
# transspec_m::Float64 # mass [kg] of atmosphere + interior
# transspec_rho::Float64 # bulk density [kg m-3] implied by r and m

# arguments
transspec_p:float = 1e2 # (INPUT) level probed in transmission [Pa]

# get the observed height
idx = int(np.argmin(np.abs(atm.p - transspec_p)))
transspec_r = atm.z[idx] + atm.planet_radius

# get mass of whole atmosphere, assuming hydrostatic
transspec_m = np.amax(atm.pl) * 4 * np.pi * atm.planet_radius**2 / atm.grav_s

# add mass of the interior component
transspec_m += atm.planet_mass

# get density of all enclosed by observed layer
transspec_rho = 3.0 * transspec_m / (4.0 * np.pi * transspec_r**3)

return transspec_rho

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