Sun's photosphere
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lowest part of the sun's atmosphere. hot gas glows and emits energy as
radiation into space.
Corona
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outermost layer of sun's atmosphere. low density, extends far. high temp,
but not hot.
, solar wind
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during an active sun, more intense solar wind from CMES is coming off the
sun, meaning more radiation to interact with our magnetosphere.
Solar constants
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granulation, spicules, solar wind
Newtons Law of Universal Gravitation
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attractive gravitational force between any two bodies. Equal but opposite
forces.
What causes seasons
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solar flux density. (energy concentration) Sunlight hitting at tilt.
Give this one a try later!
lowest part of the sun's atmosphere. hot gas glows and emits energy as
radiation into space.
Corona
Give this one a try later!
outermost layer of sun's atmosphere. low density, extends far. high temp,
but not hot.
, solar wind
Give this one a try later!
during an active sun, more intense solar wind from CMES is coming off the
sun, meaning more radiation to interact with our magnetosphere.
Solar constants
Give this one a try later!
granulation, spicules, solar wind
Newtons Law of Universal Gravitation
Give this one a try later!
attractive gravitational force between any two bodies. Equal but opposite
forces.
What causes seasons
Give this one a try later!
solar flux density. (energy concentration) Sunlight hitting at tilt.
