6 The solar emission Solar Emission Spectrum spectrum shown to the right is broad. meaning light is 4500 emited over the 4000 entire visible region of the electromagnetic spectrum, but it also has "dips" in the intensity. Search the web for "Fraunhofer lines" apd describe the cause of these 3500 3000 2500 2000 E 1500 1000 500 dips" in intensity. What specifically is the cause of the 200 400 600 800 1000 Wavelength (nm) large "dip" at-760 Intensity
6 The solar emission Solar Emission Spectrum spectrum shown to the right is broad. meaning light is 4500 emited over the 4000 entire visible region of the electromagnetic spectrum, but it also has "dips" in the intensity. Search the web for "Fraunhofer lines" apd describe the cause of these 3500 3000 2500 2000 E 1500 1000 500 dips" in intensity. What specifically is the cause of the 200 400 600 800 1000 Wavelength (nm) large "dip" at-760 Intensity
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Transcribed Image Text:6. The solar emission
spectrum shown to
the right is broad,
meaning light is
emitted over the
Solar Emission Spectrum
4500
4000
entire visible region
of the
electromagnetic
spectrum, but it also
has "dips" in the
intensity. Search the
web for "Fraunhofer
3500
3000
2500
2000
1500
1000
500
lines" and describe
the cause of these
"dips" in intensity.
What specifically is
the cause of the
large "dip" at -760
nm?
200
400
600
800
1000
Wavelength (nm)
Intensity
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