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Table 1
Parameters used in modeling.
Symbol | Quantity |
---|---|
t | Time |
tk, ![]() |
Time of lunar, planetary eclipse |
T | Observation duration |
L | Distance to the observer on Earth |
S | Star radius |
α | Binary inclination angle, w.r.t. orbital plane |
s1, s2 | Planet, moon radius |
a1, a2 | Planet, moon albedo |
R1, R2 | Planet, moon position vector |
![]() |
Binary c.m.-position vector |
![]() |
Reduced position vector |
![]() |
Arbitrary planet surface vector |
θ | Azimuth angle |
z | Vertical coordinate w.r.t. planet center |
l | Vertical displacement of shadow center |
v | Shadow velocity |
τ(l) | Eclipse duration |
ϒ(l) | Eclipse magnitude |
ν | Continuous frequency variable |
ω | Barycenter angular frequency, mean motion |
ϑ = ωt | Barycenter phase angle, mean anomaly |
Ω | Lunar orbital frequency |
φ = Ωt | Lunar phase |
![]() |
Observation direction |
θo | Observation inclination, polar angle |
ϕo | Phase at inferior conjunction, azimuth |
I(t) | Variable star luminosity |
IT(ν) | Fourier transform of star luminosity |
I0 | Average star luminosity |
F(t) | Observed reflection signal |
FT(ν) | Fourier transform of reflection signal |
f(t) = f(ϑ, φ) | Total reflected light curve |
![]() |
Fourier coefficient of light curve |
g(ϑ) | Time-integrated dip for lunar eclipse |
gn | Fourier coefficient of g |
h(ϑ) | Single-planet phase light curve |
hn | Fourier coefficient of h |
i, j, k, | Basis vectors for orbital plane |
![]() ![]() ![]() |
Basis vectors for lunar plane |
N = ωT∕2π | Number of orbits |
k | Eclipse index number |
n, m | Integer indices |
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