Elements From Stars
Foundations of Spectroscopy
Energia nuclear (2)
Objectives Explore the structure of the Sun. The Sun Describe the solar activity cycle and how the Sun affects Earth. Compare the different types of spectra.
Nuclear Reactors, BAU, 1 st Semester, 2007-2008 (Saed Dababneh). 1 Neutron Attenuation (revisited) Recall t = N t Probability per unit path length. X I0I0.
Nuclear Reactor Theory, JU, Second Semester, 2008-2009 (Saed Dababneh). 1 Neutron Attenuation Recall t = N t Probability per unit path length. X I0I0 I.
Nuclear and Radiation Physics, BAU, Second Semester, 2009-2010 (Saed Dababneh). 1 Neutron Excess Remember HWc 1. Asymmetry.
Detailed Study of the 4 He Nuclei through Response Function Separations at High Momentum Transfers Spokespersons Fatiha Benmokhtar U. Maryland, College.
Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion.
Montgomery Productions Proudly Present: The Sun. Is a star Made of gases –71% hydrogen –27% helium Is our primary source of energy –Light (radiation)
Cosmic Rays Basic particle discovery. Cosmic Rays at Earth – Primaries (protons, nuclei) – Secondaries (pions) – Decay products (muons, photons, electrons)
200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 Earth-Sun-Moon Seasons Solar System Stars Laws and.