Signature of the turbulent component of the solar dynamo on active region scales and its association with flaring activity

Obtaining observational evidence of the turbulent component solar dynamo operating in convective zone is a challenging problem because action hidden below photosphere. Here we present results statistical study flaring active regions (ARs) that produced strong flares an X-ray class X1.0 and higher during time period covered cycles 23 24. We introduced magneto-morphological classification (MMC) ARs, which allowed us to estimate possible contribution into structure AR. found 72\% cases, ARs do not comply with empirical laws global (frequently they are bipolar or, if are, violate either Hale polarity law, or Joy's leading sunspot prevalence rule), may be attributed influence inside on spatial scales typical ARs. Thus it appears governed by dynamo. A from these ARs-``violators'' enhanced second maximum descending phase cycle, when toroidal field weakens becomes more pronounced. These findings consensus concept essential role non-linearities intermittency magnetic fields generation zone, follows simulations