7
How we determine T, r, P vs depth II
•
–
•From observations of “oscillations” or “solar seismology”
–The sun oscillates like a bell (or the air in an organ pipe)
–The frequency depends upon sound speed, which depends upon T(r), r(r), P(r)
–Observations from “Global Oscillation Network Group (GONG) telescopes.
–
•From using Kirchoff’s laws
–The Sun looks like continuous emission: Solid or hot dense gas
–Absorption lines in the spectrum: Cooler gas between us and the dense gas