The Fraunhofer lines in the solar spectrum are actually: A) emission lines from

Author Question: The Fraunhofer lines in the solar spectrum are actually: A) emission lines from (Read 568 times)

plus1

Hero Member
Posts: 676

on: Aug 28, 2013

The Fraunhofer lines in the solar spectrum are actually:
A) emission lines from hot gases in the chromosphere of the Sun.
B) emission sections of the continuous spectrum of the photosphere.
C) zeeman lines around sunspots due to their strong magnetic fields.
D) absorption lines due to the thin outer layer above the photosphere.
E) red shifted lines due to the sun's rotation.

notis

Hero Member
Posts: 596

Reply #1 on: Aug 28, 2013

I know the answer! It's D.

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