On the basis of vector magnetograms of two flaring active regions (ARs
) we analyze the scaling behavior of the current helicity H-c in the p
hotosphere. The signed measure so obtained possesses a well pronounced
sign-singularity in the range of scales from more than 10(4) Km down
to the resolution limit of observations. We found that during the flar
ing process there is a signature both of a reorganization of the curre
nt helicity in the photosphere and of a strong magnetic energy dissipa
tion of the photospheric magnetic field.