00:01
Let's discuss this question.
00:02
So here we need to determine the electric field amplitude of sunlight at top of earth's atmosphere.
00:08
Also, what pressure does it exist? what is the sunlight intensity? what fraction of atmosphere pressure does this amounts to? so let's start here.
00:18
Distance, first of all is given as 1 .5 multiplied by 10 raised to 11 meter.
00:30
And here, half.
00:34
E0e square is equal to half multiplied by 1 mu not 1 divided by mu not b square.
00:44
So total energy density that is u will be equal to half e0 e square plus half multiplied by 1 divided by mu not b square is equal to e0 e square.
01:10
So intensity, i will be equal to u c that is equal to e0, e, square c that is equal to p divided by 4 .5.
01:24
So here we can say e is equal to under root p divided by 4 5e0r square c, that is equal to under root 9 multiplied by 10res to 9 multiplied by 10x to 26 divided by 1 .5 multiplied by 10 raise to 11 square multiplied by 3 multiplied by 10 raise to 8.
01:51
So here we can say e is equal to 720 .96 newton per column.
02:04
Or we can also say that e is equal to 721 newton per column.
02:11
Now further here we can say b is equal to e divided by c which will be equal to 721 divided by 3 multiplied by 10 raise to 8.
02:21
So this is equal to 2 .403 multiplied by 10 raised to minus 6 star...