Abstract

Abstract. A network of particle detectors located at middle to low latitudes known as SEVAN (Space Environmental Viewing and Analysis Network) is being created in the framework of the International Heliophysical Year (IHY-2007). It aims to improve the fundamental research of the particle acceleration in the vicinity of the Sun and space environment conditions. The new type of particle detectors will simultaneously measure the changing fluxes of most species of secondary cosmic rays, thus turning into a powerful integrated device used for exploration of solar modulation effects. Ground-based detectors measure time series of secondary particles born in cascades originating in the atmosphere by nuclear interactions of protons and nuclei accelerated in the galaxy. During violent solar explosions, sometimes additional secondary particles are added to this "background" flux. The studies of the changing time series of secondary particles shed light on the high-energy particle acceleration mechanisms. The time series of intensities of high energy particles can also provide highly cost-effective information on the key characteristics of interplanetary disturbances. The recent results of the detection of the solar extreme events (2003–2005) by the monitors of the Aragats Space-Environmental Center (ASEC) illustrate the wide possibilities provided by new particle detectors measuring neutron, electron and muon fluxes with inherent correlations. We present the results of the simulation studies revealing the characteristics of the SEVAN networks' basic measuring module. We illustrate the possibilities of the hybrid particle detector to measure neutral and charged fluxes of secondary CR, to estimate the efficiency and purity of detection; corresponding median energies of the primary proton flux, the ability to distinguish between neutron and proton initiated GLEs and some other important properties of hybrid particle detectors.

Highlights

  • High energy particles, accelerated on or near the Sun (Solar Cosmic Rays – SCR), are superimposed on the Galactic Cosmic Ray (GCR) background

  • Understanding the fundamental physical processes of particle acceleration on the Sun and by coronal and interplanetary (IP) shocks is crucial for the exploration of space

  • The size and magnetic field of IP Coronal Mass Ejections (ICMEs) are obviously correlated with the modulation effects that the ICME poses on the galactic cosmic rays during its propagation up to 1 AU

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Summary

Introduction

High energy particles, accelerated on or near the Sun (Solar Cosmic Rays – SCR), are superimposed on the Galactic Cosmic Ray (GCR) background. Ground-based detectors measure the time series of secondary particles born in cascades originating in the atmosphere by primary ions and solar neutrons.

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