Basic LTE Relations (Hubeny & Mihalas 4)

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Presentation transcript:

Basic LTE Relations (Hubeny & Mihalas 4) Planck Curve Maxwellian Velocity Distribution Boltzmann Excitation Relation Saha Ionization Equation

Planck (Black Body) Spectrum Good description of radiation field deep in the atmosphere where little leakage occurs

Planck (Black Body) Spectrum Wien’s law: peak of the λ curve in Ångstroms Stefan-Boltzman law: area under the curve, σ = 5.6705x10-5 erg s-1 cm-2 K-4

Planck curve in IDL Wave=10.*(findgen(1000)+1.) ; 10,20,…10000 Ångstroms Teff=30000. ; Kelvin B=planck(wave,teff) ; Planck function Applet at jersey.uoregon.edu/vlab

State of Gas in LTE (T, N) Maxwellian velocity distribution

Boltzmann Excitation Equation nijk = number density of atoms of excitation state i ionization state j chemical species k Χijk = excitation energy of state i relative to ground state of atom/ion, Χ0jk gijk = statistical weight (# degenerate sublevels, 2J+1) Ludwig Boltzmann

Partition Functions Dependent on T log U(T) tabulated in Gray, Appendix D.2, as function of

Saha Ionization Equation ΧI = ionization potential energy above ground state to ionize the atom Listings in Gray, Appendix D.1 Meghnad Saha

Key Variables: T, ne Hubeny & Mihalas Chap. 17 give a general iterative method to find ne from T and N, where N=total number of particles Interesting limiting cases …