A typical high-end strobe like a Canon 580 EX-II or a Nikon SB800 or SB900 has an "approximate" watt-second equivalent to about 80 watt seconds at full power. It's difficult to put a rating on it because of a number of factors.
With studio strobes, the reflector's angle of coverage plays a *HUGE* part in the exposure it will deliver. The Guide Number in the USA is almost always given at ISO 100, in Feet. In Europe, it is almost always listed in Metres, so the GN will be much lower, since a meter is about 3.1 feet.
Most studio flash makers will have specifications in Guide Number; Some makers will list their GN for their "standard" reflector, which may be a 5-inch, a 7-inch or an 8- or 8.5- inch inch reflector that covers anywhere from 105 down to as little as 55 degrees. The wider the angle of coverage, the lower the Guide Number is going to be. Some manufacturers will list their GN using an 11 or 11.5 inch reflector, which is usually a rather deep bowl-shaped reflector, often covering between 50 and 65 degrees,and usually delivering a very powerful, well-focused flash output, and usually THE MOST powerful or higher Guide Number output that flash head is capable of giving.
Paul C. Buff and the Alien Bees just got a new 11 inch long-throw sports reflector, with a narrow beam angle and a highly polished bowl. DynaLite also has a similar flash reflector for arena usage.
With portable speedlights, the Guide NUmber will also vary,hugely, depending on the beam spread; at 24mm the GN will be low, at 85mm the beam spread will be narrower and the light concentrated and the GN will be higher; the very-newest top-end flashes have gone to 105mm and even 200mm telephoto beam angles, which give a very,very narrow spread and an exceedingly high GN.
So...it's hard to put an exact number on speedlight vs studio strobe until you compare apples with apples, meaning angle of beam spreads must be similar. S, look for the Guide Number in the same units at the same ISO, 100 ISO, and only then can you get a reasonable and fair comparison.