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1Fedorov YI. The cosmic ray intensity on the initial stage of the solar flare. Russian. 2018 ;34(1):3-20.
1Fedorov YI. Cosmic ray distribution function under anisotropic particle scattering on magnetic field fluctuations. Russian. 2019 ;35(1):3-26.
1Fedorov YI. The cosmic ray distribution function on the initial stage of the solar proton event. Ukrainian. 2020 ;36(3):3-20.
1Masliukh VO, 1Hnatyk BI. Cosmic ray acceleration in Hypernova remnants expanding into wind bubbles of progenitor stars of Wolf-Rayet type. Ukrainian. 2013 ;29(5):3-24.
Megn AV. Cosmic radio sources with maximum of the emission spectral density at the decameter wavelengths (according to the Grakovo catalogue). Russian. 2008 ;24(6):413-425.
1Melekh BY, Pilyugin LS, Korytko RI. The correspondence between strong emission line intensities in the spectrum of an H II region and its chemical composition. Russian. 2012 ;28(4):56-75.
1Elyiv AA, 2Hnatyk BI. Correlation of the ultra high energy cosmic rays with different classes of extragalactic objects: contribution of the nearest and brightest members of sample. 2006 ;22(4):297-308.
1Zhdanov VI, Ivashchenko GY. Correlation function of quasars from SDSS DR3. 2008 ;24(1):3-14.
Ivashchenko GY, 1Zhdanov VI. Correlation function of quasars and redshift-space distortions from SDSS DR5 data. Russian. 2010 ;26(1):43-56.
1Kolesnyk YL, 1Shakhov BA. On coronal influence for GCR distribution in the absence of its interaction with the interstellar medium. Russian. 2015 ;31(1):32-39.

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