Movie at http://sohowww.nascom.nasa.gov/bestofsoho/Movies/dynamo/dynamosm.mpg
Slide 10
Inside the Sun
Core
Radiative Zone
Convection zone
Image at http://solarscience.msfc.nasa.gov/interior.shtml
Slide 11
The Sun’s Atmosphere
Photosphere
Chromosphere
Corona
Photosphere image: http://science.msfc.nasa.gov/ssl/pad/solar/surface.htm
Chromosphere image: http://science.msfc.nasa.gov/ssl/pad/solar/chromos.htm
Corona image: http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=191
Slide 12
Nuclear chain reaction (hydrogen forming helium)
Releases radiation (gamma rays)
The gamma ray loses energy as it bounces around inside the Sun
It is finally released at the photosphere, primarily as visible light
Slide 13
Sunspots
Dark and small (but brighter than Full Moon and big as Earth)
Cool-- temperatures only 6,200 F (Sun’s surface is 10,000 F)
Associated with magnetic fields: one set of spots is positive, other is negative
Image at http://sohowww.nascom.nasa.gov/gallery/top10/top10_results.html
Slide 14
Our Sun has an activity cycle of 11 years
Sunspots appear at specific latitudes on Sun
Bands of latitude move towards equator during cycle
Slide 15
Flares (Explosions of energy on the surface of the Sun)
Prominences
Coronal Mass Ejections (massive clouds of plasma ejected from the Sun)
Movie: Six months with EIT 171 (Aug. 12, 2003 - Feb. 9, 2004)
Slide 16
Blows charged particles and magnetic fields away from the Sun
Charged particles captured by Earth’s magnetic field
Create Auroras or Northern and Southern Lights
Slide 17
Electrons from solar wind are captured by the Earth’s magnetic field
Interact with atoms in our atmosphere: oxygen and nitrogen make red and green; nitrogen can also make violet
Northern lights are Aurora Borealis, while southern are Aurora Australis
Animation of solar wind impacting the magnetosphere and creating aurora
Slide 18