A) All Fraunhofer lines changed into bright coloured lines
B) no lines at all
C) a smaller number of dark Fraunhofer lines
D) a large number of dark Fraunhofer lines
Correct Answer: A
Solution :
We know that when the total solar eclipse occurs, the photosphere is covered. Emission lines from vapours of elements present in chromospheres appears as coloured bright lines. Therefore, all fraunhofer lines are converted into bright coloured lines.
You need to login to perform this action.
You will be redirected in
3 sec
