$\log 6.7$ means "what power do I need to raise 10 to in order to get 6.7?".
Put in another way: $10^{\log 6.7}=6.7$.
Yet another way: we have $10^x=6.7$, and the answer is $x=\log 6.7$.
Normally we can look up $\log 6.7$ in a log table or use a calculator to see what the decimal number version of $\log 6.7$ is. But what if we couldn't do that?
Okay, what if we do this:
$10^0=1$ and $10^1=10$.
$10^x=6.7$, so $x$ must be between 0 and 1.
Let's take the average: $\frac{0+1}{2}=\frac{1}{2}$. Taking the average is easy and it ensures that we end up somewhere "between" the values we're taking the average of (0 and 1 in this case).
$10^\frac{1}{2}\approx 3.16$. Okay so less than 6.7.
Let's take the average again: $\frac{1/2+1}{2}=\frac{3}{4}$
$10^\frac{3}{4}\approx 5.62$. Still less than 6.7
Let's take the average again: $\frac{3/4+1}{2}=\frac{7}{8}$
$10^\frac{7}{8}\approx 7.5$. So now we're over 6.7. Let's just take the average of $3/4$ and $7/8$ then.
Let's take the average again: $\frac{3/4+7/8}{2}=\frac{13}{16}$.
$10^\frac{13}{16}\approx 6.49$. Less than 6.7, but we're getting closer.
If we keep doing this eventually we'll get a number such that $10^{\text{number}}=6.7$. Implementing this method in Python, it took 26 iterations to get $10^{0.82607480\;13854027}=6.69999997970653$.
Wolfram alpha says $\log_{10} 6.7 = 0.82607480\;27...$.
If we wanted to do this by hand, we'd have to assume we had a method for approximating numbers like $10^\frac{13}{16}$ of course.
So just on the face of it, it seems like a lot of work to calculate logs between 0 and 1 by hand. There are better ways to approximate logs then what I've chosen in this post, but they all rely on doing a lot of calculation by hand (if you don't have a computer).
But doing a heck load of manual computations was how the first log tables were made. Napier spent 20 years making his. Log tables give you a faster and more reliable way to do multiplication - but only because someone went through the massive effort of putting together a log table in the first place.