Earth science 24.3
Our star, the Sun is a big ball of gas And it's 99 percent of our solar system's mass It's an average star in our Milky Way Warming the Earth every day.
The H-alpha radial velocities of an arch filament system in solar emerging flux region Shino Kawahara Rakutou High School KYOTO.
Overview of CMSO Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas S. Prager May, 2006.
Activities today 1.Bellwork 2.Fission/fusion Discussion 3.Think-peer share activity: Double-bubble map on Fission-fusion 4.Note taking 5.Quiz.
The Solar Corona – contd. We discussed: Physical properties of the corona We will now discuss: Coronal scale height Ionization equilibrium Coronal heating.
Space weather: solar drivers, impacts and forecasts Henrik Lundstedt Swedish Institute of Space Physics Lund We live inside the continuously expanding.
The Formation and Structure of Stars Chapter 9. The Big Picture Stars exist because of gravity. Gravity causes interstellar material to collapse to form.
C. the solar system
Lesson 7 solar system
The Sun and the Particle Physics
Fusion and Fission
