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1
MODELING THE SUN
2
THE SOLAR INTERIOR
3
HELIOSEISMOLOGY
4
SOLAR NEUTRINOS
5
THE SOLAR NEUTRINO PROBLEM
6
THE PHOTOSPHERE
7
LIMB DARKENING
8
SUPERGRANULES
9
THE CHROMOSPHERE
10
SPICULES
11
THE CORONA
12
CORONAL HEATING
13
THE SOLAR WIND
14
SUNSPOTS
15
MAGNETIC FIELDS
16
SOLAR STORMS
17
OTHER SURFACE FEATURES
18
THE SUNSPOT CYCLE
19
THE MAGNETIC-DYNAMO EFFECT
20
ORIGIN OF THE MAGNETIC FIELD
21
CONCEPT CHECK 16-17
Description:
Explore the intricate structure of our nearest star in this comprehensive astronomy lecture. Delve into the Sun's interior, examining models and helioseismology techniques used to understand its composition. Investigate the solar neutrino problem and its implications for stellar physics. Examine the Sun's visible layers, including the photosphere, chromosphere, and corona, while learning about phenomena like limb darkening, spicules, and coronal heating. Analyze solar features such as sunspots, magnetic fields, and solar storms. Understand the sunspot cycle and the magnetic-dynamo effect that drives solar activity. Gain insights into the origin of the Sun's magnetic field and its impact on space weather.

General Astronomy - The Structure of the Sun

Spahn's Science Lectures
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