Semester 1 - Formulae Flashcards
Spherical trig
sinA/a = sinB/b = sinC/c
Specific flux
Fv = (2π ∫ 0) (π/2 ∫ -π/2) Iv (θ,φ) cosθsinθdθdφ
μ and dμ
μ = cosθ
dμ = -sinθdθ
integrating factor
dy/dx + P(x)y = Q(x)
where the integrating factor is μ(x) = exp^( ∫P(x)dx)
hence the ODE becomes
d/dx (μ(x)y) = μ(x)Q(x)
intensity emitted
dIv = p jv ds
where jv is the emission coefficient
intensity absorbed/gained
dIv = -p kv Iv ds
where kv is the absorption coefficient
optical depth
dτv = pkvds
angle-dependent definition of optical depth
dτv,μ = -dτv/μ
mean intensity
Jv = 1/4π ∮ Iv dΩ
equation of transfer
μ dIv/dτ = Iv - Sv
relation between eddington flux and k integral
Hv = dKv/dτ
total momentum
dp = dEv/c cosθ
where dp is the total momentum
dEv =
IvcosθdAdΩdt
dΩ =
sinθdθdφ
Eddington approximation
K = I/3 = J/3
Eddington Barbier relation
F = π Sv
where Sv ~ Bv
equation of transfer in terms of absorption and emission coefficient
dIv/ds = p jv - pkv Iv
Source function
Sv = jv/kv
line depth
Aλ = 1 - Rλ
where Rλ = Fλ/Fc
in a naturally broadened line to find the normalisation constant.
∆v = v - v0 = 0
HWHM
HWHM = ∆v
when
I = Ipeak/2