Two parameters such as magnetic fields near the light cylinder Blc\documentclass[12pt]{minimal}
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\begin{document}$B_{lc} $\end{document} and rates of rotational energy losses dEdt\documentclass[12pt]{minimal}
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\begin{document}$\frac{dE}{dt} $\end{document} for 1795 radio pulsars without high energy emission (R), 52 radio loud gamma-ray pulsars (γ\documentclass[12pt]{minimal}
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\begin{document}$\gamma$\end{document}+R), 33 radio quiet gamma-ray pulsars (γ\documentclass[12pt]{minimal}
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\begin{document}$\gamma$\end{document}) and 61 radio loud X-ray pulsars (X+R) are compared with each other in this work. Pulsars with registered X-ray and gamma-ray emission have the higher median values of Blc\documentclass[12pt]{minimal}
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\begin{document}$B_{lc} $\end{document} and dEdt\documentclass[12pt]{minimal}
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\begin{document}$\frac{dE}{dt} $\end{document} as compared to the population of ordinary radio pulsars. There is a trend of increasing of luminosities in X-ray and gamma-ray ranges for higher values of magnetic field near the light cylinder. We hypothesize that non-thermal X-ray and gamma-ray emissions are generated near the light cylinder by the synchrotron mechanism.
