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We study the applicability of the idea of internal absorption of gamma-raysproduced through synchrotron radiation of ultrarelativistic protons in highlymagnetized blobs to 1ES 0229+200 and 3C 66A, the two TeV blazars which showunusually hard intrinsic gamma-ray spectra after being corrected for theintergalactic absorption. We show that for certain combinations of reasonablemodel parameters, even with quite modest energy requirements, the scenarioallows a self-consistent explanation of the non-thermal emission of theseobjects in the keV, GeV, and TeV energy bands.

Modeling the hard TeV spectra of blazars 1ES 0229+200 and 3C 66A with an internal absorption scenario