Electromagnetic radiation in the infra red, visible, and ultra violet frequency ranges
Our sun, Sol, uses hydrogen for fuel.
The sun's energy (and that of all other stars) comes from nuclear fusion. The nuclei of hydrogen atoms (ie protons) fuse together to produce helium and release energy.
As the ocean's waves absorb or release energy from the sun, the transfer of energy changes.
As the ocean's waves absorb or release energy from the sun, the transfer of energy changes.
As the ocean's waves absorb or release energy from the sun, the transfer of energy changes.
The sun gets its energy from the process of fusion, where hydrogen atoms are fused together in the high temperatures and pressures of the Sun's core to produce helium atoms and release energy in the form of gamma rays..
There is no volcanoes on the sun, but sometimes a large energy release known as a solar flare can be mistaken for a volcano.
It's nuclear fusion. There are several steps, but the overall reaction converts hydrogen into helium, with the release of energy.
Nuclear reaction inside the Sun is fusing of Hydrogen to Helium and release out thermal energy.
The Sun releases the energy contained in mass (Energy=Mass*the velocity of light squared) (E=MC2). As a current main sequence star the Sun uses Hydrogen as the source of mass to release this energy. It does so by fusing Hydrogen into Helium in its core.
Brief bursts of energy from the sun's photosphere are called solar flares. These are sudden flashes of increased brightness on the sun's surface that release a large amount of energy in a short period of time.
The energy stored in the sun is primarily in the form of nuclear fusion reactions occurring in its core, which release massive amounts of energy in the form of sunlight. This energy output is measured in watts per square meter at the sun's surface, rather than in degrees.