The answer is: objects above the surface of the spinning sphere do still feel some apparent equivalent of gravity, although the higher up they go, the wonkier this apparent gravity gets.
Now, there are two ways of analyzing this type of problem: the non-inertial way and the inertial way. In the non-inertial way, we think about the problem from the perspective of a reference frame that's rotating with the shell, while in the inertial way we analyze it from a reference frame that's not accelerating (to be definite, lets say the reference frame of the star). The non-inertial way works by introducing new apparent forces that come about simply by virtue of not being in an inertial frame-- in the special case of a rotating frame, these are known as the centrifugal and Coriolis forces. This way of analyzing the problem is very useful for performing calculations, but doesn't do much in the way of physical intuition, so I'll explain from the inertial frame.
In an inertial frame, everything moves according to newton's laws-- that is, stuff moves in straight lines unless something forces it not to. So, think about the problem of a person standing on the inside of the sphere and jumping. If objects not on the surface did not feel an effective force pulling them to the sphere, we would expect our unfortunate civilian to drift off towards the sun as soon as he left the ground. However, this doesn't happen. To see why, note that our test subject isn't initially sitting still with respect to our inertial frame-- he's moving with the surface of the sphere. Thus, as soon as he stops making contact with the sphere, he'll move in a straight line in our inertial frame. Note, however, that spheres aren't straight. So, he'll collide back with the sphere eventually, a process that from his point of view looks just like an effective gravity pulling him to the sphere. This is the effect of the centrifugal force, had we instead analyzed it from the non-inertial frame.
Now, remember that earlier I said that the apparent gravity gets wonkier as you jump higher? From the inertial perspective, this has to do with the fact that circles look like parabolas if you zoom in close, but not if you zoom out far enough. Meanwhile, from a non-inertial standpoint, it's due to the Coriolis force. However, whatever way you decide to analyze it, the precise answer of how wonky gravity becomes depends on how fast the sphere is spinning, how large it is, and how high up you go. If I have more time later, I'll explain this/analyze your problem in more detail.
Hopefully that helps!
ADDENDUM: Actual Calculations
First, I'd like to clarify that how wonky your pseudo-gravity gets (ie the Coriolis force) actually depends on velocity, not on how high you go. The reason I said it depended on how high you go was that for object on a ballistic trajectory (like a person jumping), travelling higher = more speed and more time for the Coriolis force to act, thus more displacement. Now the centrifugal force does vary based on height, but 1 AU is so ridiculously large that it will be constant for all intents and purposes.
Now, for actual numbers: Based off your specs of $r = 1$ AU, $a_{centrifugal} = 9.8 m/s^2$ and the equation for centrifugal acceleration $a_{cent} = \mathbf{- \omega \times (\omega \times r)}$, we find that the magnitude of the angular acceleration needed is
$$ |\omega| = 8.1 * 10^{-6} s^{-1}$$
which corresponds to a rotational period of about 9 days. Luckily, this leads to a tangential velocity of "only" $0.004c$, so we can ignore relativistic effects. Now, the equation for acceleration caused by the Coriolis effect in the non-inertial frame of the ring is
$$a_{cor} = -2 \mathbf{\omega \times v}$$
where $\mathbf{v}$ is the velocity of your object as seen in the rotating frame. Note that this means
$$|a_{cor}| \leq 2\mathbf{|\omega||v|}$$
Now, I'd guess that countering the Coriolis force for something powered like a bird or superman would be essentially imperceptible if $a_{cor}$ were less than $0.01 m/s^2$. Putting it all together, we find that the Coriolis force doesn't play a big role for things capable of generating their own movement as long as $$|\mathbf{v}| < 616 m/s$$
which is pretty fast. Now, for objects on a ballistic trajectory that can't maneuver to counter the Coriolis force, the effects can add up differently. For a rough idea of how much this will be, note that on earth,
$$|\omega_{earth}|=7.3\times10^{-5} s^{-1}$$
So, projectiles will be affected by the coriolis force a bit less (their landing displacement will be smaller by a factor of about $\sqrt{10}$) than they are on Earth.
As a final bit of analysis/buzzkill, I just want to point out that this ring would probably tear itself apart very easily. With the angular speeds and radius you're talking about, and assuming a material tensile strength of $100GPa$, which is about as much as carbon nanotubes, we find that the necessary density of the ring material has to be less than $68 g/m^3$ in order for the ring not to tear itself apart. That's nothing. Hydrogen gas is more dense than that.