Step 1: Use radiation pressure for a perfectly absorbing surface.
Since the surface is non-reflecting (perfectly absorbing), the radiation pressure is
\[
P_r=\frac{I}{c}
\]
where
\[
I=\text{energy flux (intensity)}
\]
and
\[
c=3\times10^8\,\text{m s}^{-1}.
\]
Also,
\[
P_r=\frac{F}{A}
\]
Therefore,
\[
\frac{F}{A}=\frac{I}{c}
\]
or
\[
I=\frac{Fc}{A}.
\]
Step 2: Convert the given area into SI units.
Given,
\[
A=15\,\text{cm}^2
\]
\[
A=15\times10^{-4}\,\text{m}^2
\]
\[
A=1.5\times10^{-3}\,\text{m}^2.
\]
Also,
\[
F=10^{-6}\,\text{N}.
\]
Step 3: Calculate the energy flux.
Substituting in
\[
I=\frac{Fc}{A},
\]
\[
I=\frac{(10^{-6})(3\times10^8)}
{1.5\times10^{-3}}
\]
\[
I=\frac{300}{1.5\times10^{-3}}
\]
\[
I=2\times10^5\,\text{W m}^{-2}.
\]
Step 4: Express in the given form.
\[
2\times10^5
=
20\times10^4.
\]
Therefore,
\[
I=20\times10^4\,\text{W m}^{-2}.
\]
Step 5: Final conclusion.
Hence, the energy flux of light is
\[
\boxed{20\times10^4\,\text{W m}^{-2}}
\]