Question: What is spectroscopy? (E) an observational technique to measure the brightness of light at different colors / f} a method to freeze atmospheric turbulence for

 What is spectroscopy? (E) an observational technique to measure the brightnessof light at different colors / f} a method to freeze atmosphericturbulence for better resolution {Fiji the use of CCDs to capture lightmore efficiently than with photographic film (F). an analysis of the wayin which atoms absorb and emit light Question 44 [1 point) The
Fraunhofer lines in the solar spectrum are actually: if) emission sections ofthe continuous spectrum of the photosphere. If!) emission lines from hot gasesin the chromosphere of the Sun. './-::| Zeeman lines around sunspots dueto their strong magnetic fields \\___ (\":3 absorption lines due to thethin outer layer above the photosphere \\. Question 45 (1 point) According

What is spectroscopy? (E) an observational technique to measure the brightness of light at different colors / f} a method to freeze atmospheric turbulence for better resolution {Fiji the use of CCDs to capture light more efficiently than with photographic film (F). an analysis of the way in which atoms absorb and emit light Question 44 [1 point) The Fraunhofer lines in the solar spectrum are actually: if) emission sections of the continuous spectrum of the photosphere. If!) emission lines from hot gases in the chromosphere of the Sun. './-::| Zeeman lines around sunspots due to their strong magnetic fields \\___ (\":3 absorption lines due to the thin outer layer above the photosphere \\. Question 45 (1 point) According to Wien's Law, if the surface temperature of a star is increased by a factor of 3, its peak wavelength will: .5 decrease by a factor of 9 \\ .5") increase by a factor of 3 \\ .5\") not change; Wien's law has nothing to do with peak wavelength \\ (\"\"5. decrease by a factor of 3 \\x

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