Imagine you are experimenting with a wave on a rope. Here is a nice visual: 
You need to describe everything about the wave that could be important to someone across the world so that they can recreate the EXACT wave in their lab.
First of all it should be a sine wave shape:
$$y(x,t)=\sin(????)$$
And as you said, the wave might not have a height of one, so you multiply it by a number "A" that will give you whatever maximum height and depth you desire.
$$y(x,t)=A\sin(????)$$
If your wave's peaks and valleys range from $[-3,3]$, "A" should be $3$.
Now, you need to write down the frequency of the wave in time $f$. This works exactly as it does in the first equation you learned.
It is convenient to multiply it by $2\pi$ since you plan to put it inside a sine function:
$$y(x,t)=A\sin(2\pi f t)$$
Now you measure your frequency in SPACE, by taking a picture of the wave and seeing how many wavelengths fit in a meter. You get a number $\nu$. It is important to understand that this is the cycles per unit distance, NOT unit time like before: cycles/meter not cycles per second. Now, you multiply it by $2\pi$ to stuff it into a sine function:
$$y(x,t)=A\sin(2\pi f t - 2\pi \nu x)$$
We call the $2\pi f$ the "angular frequency in time" and shorten it to $\omega$ for convenience. Notice, $\omega$ is now in radians/second not cycles per second.
We call the $2\pi \nu$ the "angular frequency in space" and shorten it to $k$ for convenience. Notice, $k$ is now in radians/meter not cycles per meter. We often call $k$ the wave number.
$$y(x,t)=A\sin(2\pi f t - 2\pi \nu x) \Rightarrow y(x,t)=A\sin(\omega t - kx)$$
Finally you need to communicate the "headstart angle" $p$ like you said. $p$ is the angle the wave starts at in it's cycle when your experiment begins:
$$y(x,t)=A\sin(\omega t - kx+ p)$$
And that's where the wave equation comes from! It contains the minimum amount of information needed to describe any regular wave.