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  1. 21 Ιουν 2022 · The sun's atmosphere has three layers: the photosphere, the chromosphere and the corona. We explore each layer in more detail here.

  2. The photosphere, chromosphere, and corona are all part of the Sun’s atmosphere. (The corona is sometimes casually referred to as “the Sun’s atmosphere,” but it is actually the Sun’s upper atmosphere.)

  3. en.wikipedia.org › wiki › SunSun - Wikipedia

    The Sun is the star at the center of the Solar System. It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light and infrared radiation with 10% at ultraviolet energies.

  4. nssdc.gsfc.nasa.gov › planetary › factsheetSun Fact Sheet - NSSDCA

    Solar Atmosphere. Surface Gas Pressure (top of photosphere): 0.868 mb Pressure at bottom of photosphere (optical depth = 1): 125 mb Effective temperature: 5772 K Temperature at top of photosphere: 4400 K Temperature at bottom of photosphere: 6600 K Temperature at top of chromosphere: ~30,000 K Photosphere thickness: ~500 km Chromosphere ...

  5. www.nasa.gov › image-article › sunThe Sun - NASA

    22 Ιαν 2013 · The solar atmosphere is made up of: the Photosphere (the visible surface of the Sun), the Chromosphere (an irregular layer above the photosphere where the temperature rises from 6000°C to about 20,000°C), a Transition Region (a thin and very irregular layer of the Sun’s atmosphere that separates the hot corona from the much cooler ...

  6. 3 ημέρες πριν · Sun - Solar Atmosphere, Radiation, Core: Although there are no fires on the surface of the Sun, the photosphere seethes and roils, displaying the effects of the underlying convection. Photons flowing from below, trapped by the underlying layers, finally escape.

  7. www.nasa.gov › image-article › layers-of-sunLayers of the Sun - NASA

    10 Οκτ 2012 · This graphic shows a model of the layers of the Sun, with approximate mileage ranges for each layer: for the inner layers, the mileage is from the sun’s core; for the outer layers, the mileage is from the sun’s surface. The inner layers are the Core, Radiative Zone and Convection Zone.

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