This preview shows page 1. Sign up to view the full content.
Unformatted text preview: and geometrical causes o be able to state Kirchoff's Laws o continuous (blackbody) spectra-- melted nail Wien's Law Stefan-Boltzmann Law LT: Blackbody Radiation, NAAP Lab 3 o emission spectra make use of a hydrogen atom energy level diagram o LT: Light and Atoms (in class Wednesday) Doppler Shift o LT: Doppler Shift Characteristics of the Sun o general facts: composition, temperatures, comparison to other stars o know the 3 layers of the solar atmosphere and their characteristics o describe manifestations of solar activity: sunspots, prominences and flares Solar Energy o understand the binding energy per nucleon diagram o understand how the proton-proton reaction works o mechanisms of thermal transport (worksheet) o hydrostatic equilibrium...
View Full Document
- Fall '10