The Sun’s effect Flashcards
What are Magnetic fields are created by?
moving charges (electrons) in the sun: convection layer
Solar dynamo
converting kinetic energy into electricity
Differential rotation
rotation rate of the plasma varies with solar latitude
Zeeman effect
split spectral lines because of a magnetic field
Heliosphere
sphere of magnetic influence of our star
Solar cycle
11 year cycle of the sun, can be tracked with sunspots
Solar prominence (filaments)
Sunspots often occur in pairs linked by magnetic field line. Gas of chromosphere becomes trapped along the Closed field lines
Solar Wind
Particles from the Sun can escape the star where magnetic field lines are open (do not connect)
Typical solar wind speeds = 400 km/s (1 million mph)
Coronal holes
are where the solar wind escapes
What is the structure of the Sun’s layers?
Core Radiative zone Convective zone Photosphere Chromosphere Corona
Hydrostatic equilibrium
Gravitate pushing in Sun, And the pressure pushing out is equal. Making it stable (+) + (-) =0
Solar maximum
peak number of sunspots
Solar minimum
lowest number of sunspots
Aurora
Molecules in Earth’s atmosphere are excited by solar wind particles causing them to emit light
Aurora borealis and Aurora australis
Aurora borealis (Northern lights) Aurora australis (Southern lights)