... So how could there be a much hotter corona above the cooler photosphere? ... lines in front of the solar disk, they would "drown" in the strong background light from the solar 'surface' (the photosphere ...
... So how could there be a much hotter corona above the cooler photosphere? ... lines in front of the solar disk, they would "drown" in the strong background light from the solar 'surface' (the photosphere ...
... So how could there be a much hotter corona above the cooler photosphere? ... lines in front of the solar disk, they would "drown" in the strong background light from the solar 'surface' (the photosphere ...
... So how could there be a much hotter corona above the cooler photosphere? ... lines in front of the solar disk, they would "drown" in the strong background light from the solar 'surface' (the photosphere ...
... The spectral lines from the Sun appear as dark bands because they represent the wavelengths of light that has been absorbed by the Sun's photosphere as it emerges from deeper within it. ...
... The spectral lines from the Sun appear as dark bands because they represent the wavelengths of light that has been absorbed by the Sun's photosphere as it emerges from deeper within it. ...
... The spectral lines from the Sun appear as dark bands because they represent the wavelengths of light that has been absorbed by the Sun's photosphere as it emerges from deeper within it. ...