1.Slope of the radial distribution of secondary muons and hadrons in EAS at PeV energy
2.Imprint of the atmospheric attenuation process on electron distribution in EAS
3.Searching for PeV neutrinos from photomeson interactions in magnetars
4.Estimation of Shape Parameter of the Radial Distribution of Cosmic Ray Shower Particles
5.Determination of the mass and energy of primary cosmic rays above 100 TeV
6.Newly Born Extragalactic Millisecond Pulsars as Efficient Emitters of PeV Neutrinos
2.Imprint of the atmospheric attenuation process on electron distribution in EAS
3.Searching for PeV neutrinos from photomeson interactions in magnetars
4.Estimation of Shape Parameter of the Radial Distribution of Cosmic Ray Shower Particles
5.Determination of the mass and energy of primary cosmic rays above 100 TeV
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