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Table H.1

List of the symbols used throughout this work and their designations in order of introduction.

Symbol Designation

i imaginary number
real part
imaginary part
conjugate
associated with the Earth
associated with Venus
RET planetary equatorial rotating frame
X E , Y E , Z E vectorial basis associated with RET
r radial coordinate
θ colatitude
ϕ east longitude
δ latitude/fluctuations
e r , e θ , e ϕ spherical vectorial basis
t time
g gravity
Ω planet spin vector
Ω angular velocity
R planet radius
atm associated with the atmosphere
gr associated with the ground
R atm external radius of the atmosphere
H atm typical thickness of the atmosphere
M molar mass of the atmosphere
p pressure
ρ density
T temperature
p 0 background pressure distribution
ρ 0 background density distribution
T 0 background temperature distribution
C 0 background molar concentration distribution
Γ1 adiabatic exponent
N Brunt-Väisälä frequency
RGP perfect gas constant
Rs specific gas constant of the atmosphere
U gravitational tidal potential
J tidal heating power per unit mass
V tidal velocity field
V r , V θ , V ϕ components of V in spherical coordinates
ξ displacement vector
ξ r , ξ θ , ξ ϕ components of ξ in spherical coordinates
δp tidal pressure perturbation
δρ tidal density perturbation
δT tidal temperature perturbation
c s sound velocity
κ atmospheric parameter
φ rad radiated power per unit mass
σ 0 radiation frequency
S Stefan-Boltzmann constant
ϵ a effective molar attenuation coefficient
f any perturbed quantity
σ tidal frequency
ν spin parameter
m longitudinal degree
y pressure perturbation divided by ρ0
ξ H horizontal displacement
operator associated with θ-components
operator associated with ϕ-components
m,ν Laplace’s tidal operator
n meridional degree
Hough functions
eigenvalues of Laplace’s tidal equation
components of J
components of U
components of ξr
components of ξθ
components of ξϕ
components of Vr
components of Vθ
components of Vϕ
components of δp
components of δρ
components of δT
components of y
A 1 , A 2 , A 3 coefficients of the equation r2ξr;n
B 1 , B 2 , B 3 coefficients of the equation yn
A,B,C coefficients of the vertical structure
equation
function of the variable change
vertical wavenumber
L V;n scale of variation
ε s;n acoustic coefficient
σ s;n acoustic frequency
coefficients of polarization relations
K curv curvature term in polarization relations
linear operator associated with the vertical
structure
components of the operator
associated with f
X n vector of the forcings
Y n vector of the response
σ diff;n diffusive frequency
G gravitational constant
l degrees of Legendre polynomials
associated Legendre functions
normalized associated Legendre functions
potential induced by the tidal response
components of projected on the
components of projected on the
first component of
second component of
Love numbers for the gravitational potential
coefficients of Kaula’s expansion
density expansion coefficient for the perturbation
projected on the
components of
weighting coefficients of modes in
the expansion of the tidal torque
M S mass of the star
a semi-major axis
ε obliquity
n orb mean motion
σ SD semidiurnal tidal frequency
U 2,2,2,0,0 semidiurnal gravitational tidal potential
J 2,2,2,0,0 semidiurnal thermal forcing
expansion function of the thermal forcing
projected on P2
V volumetric domain of the atmosphere
tidal torque
frequency components of the tidal torque
Δϕ phase lag of the tidal response
H associated with the horizontal component
V associated with the vertical component
grav caused by the gravitational forcing
therm caused by the thermal forcing
torque due to the horizontal component
torque due to the vertical component
factor in the expressions of the torque
z altitude
x altitude normalized by the pressure height scale
x atm normalized upper boundary
a RE;T local acceleration in the reference frame
a c centrifugal acceleration
h n equivalent depth
h c characteristic depth of the vertical wavenumber
ς n scale ratio in the vertical wavenumber
Δ discriminant in and
A,B functions generating the analytic solution
coefficients of the upper boundary equation
x crit typical damping depth
parameters
parametrized function of the analytic solution
orbital period
γ lag angle
dimensionless constant
a,b empirical parameters in the model of
Correia et al. (2003)
vertical wavenumber in CL70
η relative difference between and kCL;n
λ wavelength of light
I S;λ spectral radiance of the star
I S black-body stellar flux
R S star radius
T S surface temperature of the star
d star-planet distance
c speed of light in vacuum
h Planck constant
k B Boltzmann constant
A atm;λ albedo of the atmosphere for the wavelength λ
I 0;λ effective incident flux
l linear spatial coordinate
inc caused by the incident flux
ref caused by the reflected flux
rad caused by the flux emitted by the surface
C G molar concentration of an absorbing gas
ε G;λ molar extinction density coefficient
I λ heat power flux
J heat power per unit volume
τ λ optical depth
α λ global absorption coefficient
A gr;λ albedo of the ground for the wavelength λ
T gr surface temperature
ψ angle to the star-planet direction
I gr;BB black-body emission of the ground
ϵ gr emissivity of the ground
ϵ atm emissivity of the atmosphere
ϵ effective emissivity of the ground
T gr;0 surface equilibrium temperature
δ T gr surface temperature fluctuations
transfer function of the ground
Q atm diffusive power flux in the atmosphere
Q gr diffusive power flux in the ground
k atm thermal conductivity of the atmosphere
k gr thermal conductivity of the ground
K atm vertical turbulent thermal diffusivity
K gr thermal diffusivity of the ground
c atm thermal capacity of the atmosphere
c gr thermal capacity of the ground
skin thickness in the atmosphere
skin thickness in the ground
ς gr radiative impedance of the ground
β atm thermal conductive capacity of the atmosphere
β gr thermal conductive capacity of the ground
σ bl typical frequency of the atmospheric boundary
layer
vertical damping coefficient in the boundary layer
δ T bl temperature fluctuations in the boundary layer
associated with visible light
associated with the infrared
N number of points of the spatial discretization
T timescale of the spin evolution
M mass of the atmosphere
χ tidal frequency divided by the mean motion

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