THERMODYNAMICAL PROPERTIES AND QUASI-LOCALIZED ENERGY OF THE STRINGY DYONIC BLACK HOLE SOLUTION.

In this paper, we calculate the heat flux passing through the horizon TS|rh and the difference of energy between the Einstein and Mailer prescription within the region M, in which is the region between outer horizon H+ and inner horizon H-, for the modified GHS solution, KLOPP solution and CLH solution. The formula EEinstein=Møller|M --∑∂M TS is obeyed for the mGHS solution and the KLOPP solution, but not for the CLH solution. Also, we suggest a RN-like stringy dyonic black hole solution, which comes from the KLOPP solution under a dual transformation, and its thermodynamical properties are the same as the KLOPP solution. [ABSTRACT FROM AUTHOR]