We introduce a new experimental method for solar hadronic axions search .
It is suggested that these axions are created in the Sun during M1 transition between the first thermally excited level at 9.4 keV and the ground state in ^ { 83 } Kr .
Our method is based on axion detection via resonant absorption process by the same nucleus in the laboratory .
We use proportional gas counter filled with krypton to detect signals for axions .
With this setup , target and detector are the same which increases the efficiency of the experiment .
At present , an upper limit on hadronic axion mass of 5.5 keV at the 95 \% confidence level is obtained .