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In this paper the anomalous intense pulse of the PSR J0953+0755 was studiedin decametre wavelength range. For this pulse two scales of fine structure werediscovered. The long-scale structure consists of four components, where thevisible dispersion measures of even and odd components are different. Theobtained time-scale of the short fine structure is 1 ms. The difference invisible dispersion measure can be caused by propagation of two normal modes ofthe pulsar radiation and irregularities of electron concentration in the spacenear the neutron star like upper layers of magnetosphere and pulsar wind.

Detection of the fine structure of the pulsar J0953+0755 radio emission in the decametre wave range