rasp said:
How does the actual size of all space (in linear distance dimensions) relate to the observable universe's event horizon?...
I take by actual size in linear distance dimensions you mean in terms of distance
now at this moment----if you could temporarily freeze expansion so as to provide an opportunity to carefully measure distances by radar or some other conventional yardstick.
The observable part of the universe is normally considered to be a ball with us as center and radius about 45 billion lightyears. That is, the most distant matter from which we are now receiving light is today (partly because of expansion) slightly over 45 billion lightyears from us in actual distance.
That means if you could freeze expansion it would, starting today, take 45 billion years for a signal from us to reach that matter. We are seeing that matter (as it was over 13 billion years ago when it emitted the light) whenever we map the cosmic microwave background.
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Since you are new to the board (*welcome* by the way!) maybe I should say that astronomers call the actual distance to an object at some given time (freezing expansion at that moment) its
proper distance.
There is no simple relation between proper distance and light "travel time", because the rate of expansion has changed a lot in the past.
The jargon term astronomers use for this 45 billion lightyear distance is the "particle horizon". If shortly after the start of expansion our matter had sent out a particle at the speed of light then that particle would now be 45 billion lightyears from us (because of the combined effects of both expansion and the particle's own speed.)
The particle horizon is normally what is called the radius of the observable universe.
That is probably more than enough jargon

So let's get to your main question.
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The standard model cosmology that astronomers use comes in two flavors---infinite space and finite space.
The simplest finite space case is where there is a very slight positive curvature so that space closes on itself like the 3D analog of the 2D surface of a balloon.
The most recent authoritative complete set of cosmo data I know was published January 2009 and is called the WMAP5 data (the 5th year report from a certain NASA mission that measured cosmo parameters the most accurately so far.)
Essentially what they said is that (of course it could be the infinite space case but) in the simple finite case the radius of curvature would be at least 100 billion lightyears, so that the circumference would be at least 2 pi times that---in other words in round numbers at least 600.
That means if you could freeze expansion at this moment, and would set out at the speed of light, like a lightbeam pointed in some direction, it would take you at least 600 billion years to make the full circuit and get back home. But probably more.
We don't have a better estimate, but that gives something to compare with the figure of 45 billion lightyears for the particle horizon.