These effects are pretty easy to calculate. It turns out they both depend on exactly the same quantity, v2/c2 = GM/rc2, where v is the orbital velocity. For the SR effect, the time slowdown is sqrt(1 - v2/c2) ~ - v2/2c2. For the GR effect, the apparent speedup comes from the Schwarzschild metric ds2 = (1-2GM/rc2) dt2, which implies an approximate speedup ~ GM/rc2.
On the face of it, both effects increase as 1/r as you get closer to Earth. However GR loses as you go down, because you need to compare the slowdown in orbit vs the slowdown on the ground, which modifies the answer by an extra factor Δr/r. GR is comparable for the GPS satellites because they are in a very high orbit: 20,000 km, or about three Earth radii. Low Earth orbit would mean an altitude about 50 times less than this, so GR will be 50 times smaller for your average satellite.