Download presentation
Presentation is loading. Please wait.
1
The Sun I
2
The Sun as a model for stars and astrophysics in general
3
Close-up of a G2 Main Sequence Star
4
The Solar Interior…the prime application of the equations of stellar structure
5
Density in the solar interior
6
Temperature in the Solar Interior
7
The “Faint Young Sun Paradox”
8
Tests of Stellar Interior Models
Mass, luminosity, temperature of Sun and stars Solar neutrinos Helioseismology (and asteroseismology)
9
Helioseismology: Eigenmodes of the Sun
10
Solar Neutrino Experiments
11
Layers of the Solar Atmosphere
Photosphere Chromosphere Corona
12
Granules in the Solar Atmosphere
13
The Solar Spectrum and the Photospheric Opacity Mechanism
Similar presentations
© 2024 SlidePlayer.com. Inc.
All rights reserved.