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1Zhdanov VI, Ivashchenko GY. Correlation function of quasars from SDSS DR3. 2008 ;24(1):3-14.
1Malovichko PP. Correlation of longitudinal currents with Alfven waves generation at the solar atmosphere. 2007 ;23(5):259-265.
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.
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.
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.
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.
1Fedorov YI. The cosmic ray distribution function on the initial stage of the solar proton event. Ukrainian. 2020 ;36(3):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 intensity on the initial stage of the solar flare. Russian. 2018 ;34(1):3-20.
1Elyiv AA, 2Hnatyk BI. Cosmic ray spectrum formation in the ultra-high energy region: the effect of intergalactic magnetic field and expected contribution from individual sources. 2007 ;23(2):83-94.

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