The rate of energy emitted by an ideal surface, frequently called a blackbody, is given by the following relationship: E = K. sb. T. 4. where T is absolute temperature & K. sb
http://wiki.answers.com/Q/What_is_Stefan_Boltzmann...

( ′shte′fän ′bōlts′män ′lö ) (statistical mechanics) The total energy radiated from a blackbody is proportional to the fourth power
http://www.answers.com/topic/stefanboltzmannlaw

The total energy radiated in watts per square metre is proportional to
http://www.chacha.com/question/whatisthestefan%...

Stefan Boltzmann's law states E ~ T^4. So if there is 3000 times more energy beamed upon the earth, the temperature has to rise to radiate the energy away. En is new energy flux,
http://answers.yahoo.com/question/index?qid=201210...
