radiation balance
The amount of available energy that can be used to promote change and do work is called free energy. This is the energy that is available to do useful work in a system.
The average amount of energy of motion of each particle of a substance is called kinetic energy. It is related to the speed and mass of the particles.
The total amount of energy in an object is called energy, regardless of its form (heat, thermal, electrical, etc.).
Energy of motion is called kinetic energy.
The amount of unusable energy in a system is called entropy. Entropy measures the level of disorder or randomness in a system and represents the energy that cannot be converted into useful work.
radiation balance
radiation balance
When the amount of energy received from the sun and the amount of energy returned to space are about equal, it is called "radiative equilibrium." This balance is crucial for maintaining a stable climate, as it indicates that the Earth's energy budget is in balance, preventing significant warming or cooling over time.
radiation balance
Describe how net energy deffers from energy returned?
The amount of available energy that can be used to promote change and do work is called free energy. This is the energy that is available to do useful work in a system.
This energy is the activation energy.
It's the amount of energy given out by the sun, and the energy received by the earth. Within that is the energy reflected and the energy given off from the earth.
The average amount of energy of motion of each particle of a substance is called kinetic energy. It is related to the speed and mass of the particles.
The amount of energy available to do work after a chemical reaction has occurred is called free energy or Gibbs free energy. It represents the maximum amount of useful work that can be obtained from a system at constant temperature and pressure.
The total amount of energy in an object is called energy, regardless of its form (heat, thermal, electrical, etc.).
The Sun radiates its energy in every direction. The amount of energy received per square meter of exposed surface will decrease by the square of the distance. So, if you double the distance, the amount of energy received will be reduced to one-fourth; if you triple the distance, the energy will be reduced to one ninth.