Are you sure about that?
Many small waves are rather different from one big tsunami... and that's assuming the little ones still retain enough mass to even make it to the surface, as opposed to burning up in the atmosphere.
A lot of it also depends on the shape, velocity, and composition of the a meteor. What causes an explosion (such as the Tunguska blast) is compression of the atmosphere in front of the meteor. This in turn causes extreme heat (PV=nRT, where PV rises), rather than friction.
If a long elliptical meteor came into the atmosphere roughly parallel with the atmospheric plane (ie, long side first), it would most likely break up. However, if it came in perpendicular (ie, end first), there's a lot less surface area being compressed, and may be more likely to actually impact before bursting.
Similarly, since different compositions will have greater or lesser resistance to heat, they will fragment differently.
Velocity also plays a role; the faster a meteor is travelling, the more dramatic the compression will be. This is because velocity (not acceleration) affects the force placed upon the atmosphere through fluid dynamic equations. Additionally, the angle of impact matters as well.
A rough back of the napkin calculation: most meteors are stony, with a density of roughly 3.5 g/cm^3. Given a mass of 1000 tons = about 900 million grams, and substituting those in for volume to find the radius of a sphere... you get a sphere of with a radius of 395 cm, or roughly 8 meters in diameter. That's still large enough to cause some pretty serious damage. If you explode the meteor and say even 1% enter Earth and explode in air versus on the ground you're still looking at roughly 10 square miles of destruction total, based on impact craters of similar size.
Not to worry though, because it's highly unlikely a meteor of significant size will strike Earth.