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phys: fix solar radiation latex alignment

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eggy 2021-04-08 20:31:02 -04:00
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docs/sph4u7.md
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@ -462,7 +462,7 @@ $$P=e\sigma AT^4$$
In problems where the environment temperature is **different** from the temperature of an object, there will be power loss. The net power emitted by a body will be:
$$P_\text{net}=e\sigma A(T_1^4-T_2^4)$$
The solar radiation reaching earth is equal to $\pu{S=3.9\times10^{26} W}$ with the assumption that it is a black body.
The solar radiation reaching earth is equal to $\pu{S= 3.9\times10^{26} W}$ with the assumption that it is a black body.
### Albedo