Solar Interior (continued) Role of convection energy transport in the solar interior 1.
REVISION LECTURE I SOLAR PHYSICS PHAS M314/SPCEG012 April 23, 2012 1.
The sun
Gravitational lensing characteristics of the transparent sun
2. the sun.2
spacephysics
Skript Astrophysics
Chapter 16: The Sun. 16.1Physical Properties of the Sun 16.2The Solar Interior SOHO: Eavesdropping on the Sun 16.3The Sun’s Atmosphere 16.4Solar Magnetism.
Copyright © 2010 Pearson Education, Inc. Chapter 9 The Sun.
Lithium abundance in the globular cluster M4: from the Turn-Off up to the RGB Bump Collaborators: M. Salaris (University of Liverpool, UK) L. Lovisi, F.R.
Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q= 0.27/26.73 = 1% ppIII loss: 28% Total loss: 2.3%
1 Trieste 23-25 Sept. 2002. 2 Standard and non-standard solar models Success of stellar evolutionary theory Basic inputs of the theory Standard solar.
