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The sun emits a wide range of electromagnetic radiation across the spectrum, from radio waves to gamma rays. Different layers and processes on the sun produce various types of radiation, which contribute to the overall electromagnetic spectrum that reaches Earth. Measurements of solar radiation across the spectrum help scientists understand the sun's behavior and its effects on various processes on Earth.

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Is the spectrum of white light from the sun continuous?

Yes, the spectrum of white light from the sun is continuous, containing all colors of the rainbow. This continuous spectrum is due to the sun emitting light across a wide range of wavelengths.


Where does the peak wavelength emitted by the Sun fall in the electromagnetic spectrum?

The peak wavelength emitted by the Sun falls in the visible spectrum, specifically in the green part of the spectrum around 500 nm. This is why the Sun appears yellow-white to our eyes.


What causes the creation of Fraunhofer lines in the Sun's electromagnetic spectrum?

Fraunhofer lines in the Sun's electromagnetic spectrum are caused by the absorption of specific wavelengths of light by elements in the Sun's atmosphere. These elements absorb light at certain frequencies, creating dark lines in the spectrum that help scientists identify the composition of the Sun.


Which type of spectrum is produced when white light from the Sun passes through a prism?

A continuous spectrum is produced when white light from the Sun passes through a prism. This spectrum contains all the colors of the rainbow without any distinct lines or bands.


How does atomic spectrum differ from solar spectrum?

Atomic spectrum is produced when atoms emit or absorb light at specific energies, creating distinct lines or bands. Solar spectrum is the continuous spectrum of light emitted by the Sun, containing all wavelengths of light. Solar spectrum is produced by many elements and compounds in the Sun's atmosphere, creating a broad, continuous range of colors.

Related Questions

Which type of spectrum does the sun emit?

The sun emits a continuous spectrum, which includes all wavelengths of light across the electromagnetic spectrum. This spectrum results from the thermal radiation of the sun's surface.


Does the sun give off a discontinuous spectrum?

No. The sun gives off a full continuous spectrum.


What spectrum does the sun emit?

The Sun emits radiation across almost the entire electromagnetic spectrum.


How a star is similar to the sun if it has the same absorption lines in its spectrum that occur in the sun spectrum?

because they will have the same elements in the atmosphere...


What color is your Sun?

The sun emits all colors of the spectrum.


Is the spectrum of white light from the sun continuous?

Yes, the spectrum of white light from the sun is continuous, containing all colors of the rainbow. This continuous spectrum is due to the sun emitting light across a wide range of wavelengths.


Where does the peak wavelength emitted by the Sun fall in the electromagnetic spectrum?

The peak wavelength emitted by the Sun falls in the visible spectrum, specifically in the green part of the spectrum around 500 nm. This is why the Sun appears yellow-white to our eyes.


What spectrum is filterd in the ozone layer?

The sun rays consist of various spectrum of rays. Among them UV spectrum is filtered.


Which type of spectrum is produced when light from the sun passes through a prism?

It is the spectrum of visible light, which has the colors of the rainbow.


What type of spectrum do we see from the sun?

some of the light from the corona produces a continuous spectrum that lacks absorption lines. however the type is absorption spectrum


What is the G2 spectrum yellow dwarf called?

The G2 spectrum yellow dwarf is called the Sun.


What causes the creation of Fraunhofer lines in the Sun's electromagnetic spectrum?

Fraunhofer lines in the Sun's electromagnetic spectrum are caused by the absorption of specific wavelengths of light by elements in the Sun's atmosphere. These elements absorb light at certain frequencies, creating dark lines in the spectrum that help scientists identify the composition of the Sun.