Is there an orbit that could cause regular debris showers like in the movie Gravity? [some spoilers]

If you were in the ISS and orbiting the Earth roughly every 90 minutes, would it be possible for debris to be orbiting such that it passes you every 90 minutes?

While Neil DeGrass Tyson pointed out scientific flaws in the movie on twitter, he praised many things the movie got right in interviews, including "The 90-minute orbital time for objects at that altitude."  I think I recall an interview on a podcast that I can't remember where he specifically said that referring to the debris recurring every 90 minutes.

In reality wouldn't the debris have to be in a different orbit?  If the ISS orbits every 90 minutes (92.87 really but I'm saying 90) then after 90 minutes they would be in the same relative position.  The Earth would have rotated in the mean time so they wouldn't be over the same point on Earth, but they would be in the same position in orbit about the Earth.  Is there an orbit that would allow the same debris to cross the same spot in their orbit every 90 minutes?  Would it be nearly the same orbit, just inclined slightly?  Would that explain why the debris was moving so slowly relative to the ISS as well?

note:

There are problems with the orbits and location in the movie, I simplified my question to ask about the particular orbit of the ISS.
If I understand you correctly (and I haven't seen the movie ^_^), you want to know if it is possible for two different objects in orbit to come close to each other periodically, with roughly the same period as one of the object's orbital period. 

Yes, that is possible, but not probable.


Obviously, if the objects are in the same orbit, they are always close to each other 
If they are in slightly different orbits, one of the objects will seem to move about the other object in regular or irregular patterns, depending on orbit specifics
If they are in completely different orbits, the necessary conditions are 


the orbital period of both is equal
they have at most 1 point in common (or at least very closely approach each other)
the phasing of both objects is such that the objects are in the close approach region at the same time.



In ordinary two-body Keplerian celestial mechanics, an orbit's semi-major axis is the only orbital element that determines the orbital period. Therefore, one orbit may be circular and the other elliptic and inclined in all sorts of ways, but as long as the semi major axis of both is the same, they will have the same period. 

However, this whole scenario is completely unstable for any real-world celestial body. The (relatively small) asphericity of the Earth, as well as the presence of the Moon for example, causes all orbits around it to drift in some way or another. If you put two objects in orbits like you describe, they will not likely meet up very often before never seeing each other again for centuries.