Our Home Planet Earth is an ocean planet. Our home world's abundance of water -- and life -- makes it unique in our solar system. Other planets, plus a few moons, have ice, atmospheres, seasons and even weather, but only on Earth does the whole complicated mix come together in a way that encourages life -- and lots of it.
Short Description: Students will compare the amount of energy dissipated by an aurora in the northern hemisphere, with the record Kp index of magnetic storm severity.
Short Description: Students will use data from the IMAGE satellite to see if there is a correlation between aurora and other phenomena in the solar and geospace environment which can cause them to brighten.
Short Description: Students will use data from the IMAGE satellite to order an auroral image in time, describe how an aurora changes over time, construct a timeline of auroral changes, and compare magnetic storms for common auroral elements.
Short Description: Students explore the idea that changes in the magnetic field in the magnetotail region cause releases of energy that eventually supply the battery to light up the aurora on Earth.
Short Description: Students will algebraically solve distance equations to explain how the distance to the magnetopause balance point depends on the solar wind pressure.
Short Description: Students will use models to learn how Earth's magnetic field protects us from polar storms. They will also describe the shape of the Earth's magnetic field in space and learn its correct name.
Short Description: This activity shows the relationship between electricity and magnetism, how the Earth's magnetic field can effect (and sometimes interrupt) the flow of electricity from power companies to consumers.
Short Description: Students will compare the amount of energy dissipated by an aurora in the northern hemisphere, with the record Kp index of magnetic storm severity.
Short Description: Students will use data from the IMAGE satellite to see if there is a correlation between aurora and other phenomena in the solar and geospace environment which can cause them to brighten.
Short Description: Students will use data from the IMAGE satellite to order an auroral image in time, describe how an aurora changes over time, construct a timeline of auroral changes, and compare magnetic storms for common auroral elements.
Short Description: Students explore the idea that changes in the magnetic field in the magnetotail region cause releases of energy that eventually supply the battery to light up the aurora on Earth.
Short Description: Students will algebraically solve distance equations to explain how the distance to the magnetopause balance point depends on the solar wind pressure.
Short Description: Students will use models to learn how Earth's magnetic field protects us from polar storms. They will also describe the shape of the Earth's magnetic field in space and learn its correct name.
Short Description: This activity shows the relationship between electricity and magnetism, how the Earth's magnetic field can effect (and sometimes interrupt) the flow of electricity from power companies to consumers.