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  2. Radiative cooling - Wikipedia

    en.wikipedia.org/wiki/Radiative_cooling

    The Earth-atmosphere system is radiatively cooled, emitting long-wave radiation which balances the absorption of short-wave (visible light) energy from the sun. Convective transport of heat, and evaporative transport of latent heat are both important in removing heat from the surface and distributing it in the atmosphere.

  3. Thermal radiation - Wikipedia

    en.wikipedia.org/wiki/Thermal_radiation

    Radiation waves may travel in unusual patterns compared to conduction heat flow. Radiation allows waves to travel from a heated body through a cold non-absorbing or partially absorbing medium and reach a warmer body again. [14] An example is the case of the radiation waves that travel from the Sun to the Earth.

  4. Heat transfer - Wikipedia

    en.wikipedia.org/wiki/Heat_transfer

    The process of heat transfer from one place to another place without the movement of particles is called conduction, such as when placing a hand on a cold glass of water—heat is conducted from the warm skin to the cold glass, but if the hand is held a few inches from the glass, little conduction would occur since air is a poor conductor of heat.

  5. Black-body radiation - Wikipedia

    en.wikipedia.org/wiki/Black-body_radiation

    The law was formulated by Josef Stefan in 1879 and later derived by Ludwig Boltzmann. The formula E = σT 4 is given, where E is the radiant heat emitted from a unit of area per unit time, T is the absolute temperature, and σ = 5.670 367 × 10 −8 W·m −2 ⋅K −4 is the Stefan–Boltzmann constant. [28]

  6. An unusual object has been releasing pulses of radio waves in ...

    www.aol.com/news/unusual-object-releasing-pulses...

    An unusual object has been releasing pulses of radio waves in space for decades. ... an object 15,000 light-years from Earth in the Scutum constellation. ... magnetars release energy in a matter ...

  7. Heat transfer physics - Wikipedia

    en.wikipedia.org/wiki/Heat_transfer_physics

    The macroscopic energy equation for infinitesimal volume used in heat transfer analysis is [6] = +, ˙, where q is heat flux vector, −ρc p (∂T/∂t) is temporal change of internal energy (ρ is density, c p is specific heat capacity at constant pressure, T is temperature and t is time), and ˙ is the energy conversion to and from thermal ...

  8. Outgoing longwave radiation - Wikipedia

    en.wikipedia.org/wiki/Outgoing_longwave_radiation

    The growth in Earth's energy imbalance from satellite and in situ measurements (2005–2019). A rate of +1.0 W/m 2 summed over the planet's surface equates to a continuous heat uptake of about 500 terawatts (~0.3% of the incident solar radiation).

  9. Underwater heat waves could be reshaping the weather around ...

    www.aol.com/weather/underwater-heat-waves-could...

    The marine heat wave in the Gulf of Mexico could continue to influence the weather into the upcoming hurricane season. "The overall weather pattern combined with the warm waters could spin up a ...