About the necessity of new small EAS experiments at observation levels 500 - 600 g cm-2.

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Cosmic Rays: Air Showers, Cosmic Rays: Energy Spectra, Cosmic Rays: Composition

Scientific paper

New small EAS experiments at observation levels 500 - 600 g cm-2 devoted to investigation of the primary mass composition and energy spectrum at energies 104 - 105GeV are necessary to carry out calibration between the direct (balloons and satellites) and indirect (EAS) methods for primary cosmic flux studies. A new shower selection has to be used to apply compact EAS arrays for unbiased primary mass composition and energy spectrum estimations.

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