armen hovhannisyan

The Behavior of the Mean Multiplicity Coefficients of ASEC

Neutron Monitors During Thunderstorm Activity

Armen Hovhannisyan

Aragats Neutron Monitor

3 Dead Times of Neutron Monitor

Mean Multiplicity Coefficient

1

1

M

mmM

mm

mNm

N

0.4

1250

1,3i

ii

Nm i

N

0.004±1.207m

Nucleon double counting effect

Correlation Matrix of ArNM – Dead Time 1250mcs

Det 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18

1 * 14 2 -1 -4 5 0 -5 -4 -1 -3 2 4 2 1 3 3 -4

2 14 * 12 3 2 -1 0 -1 -4 -4 -4 -1 4 0 -1 1 2 4

3 2 12 * 10 5 -3 0 5 1 -1 -1 0 -2 1 -6 -2 -2 2

4 -1 3 10 * 10 7 5 9 0 -1 -2 0 -2 2 -4 -1 0 -2

5 -4 2 5 10 * 16 3 0 3 -1 -5 -1 1 -2 1 1 2 4

6 5 -1 -3 7 16 * 6 -1 1 -3 -1 6 -1 1 4 -1 0 2

7 0 0 0 5 3 6 * 15 10 1 3 -3 3 -5 2 -1 1 4

8 -5 -1 5 9 0 -1 15 * 19 6 1 1 -2 1 1 -1 -1 4

9 -4 -4 1 0 3 1 10 19 * 11 7 3 -1 -7 0 1 2 0

10 -1 -4 -1 -1 -1 -3 1 6 11 * 11 1 3 1 1 -2 2 0

11 -3 -4 -1 -2 -5 -1 3 1 7 11 * 15 3 -4 0 -1 0 0

12 2 -1 0 0 -1 6 -3 1 3 1 15 * 5 3 4 -2 0 -1

13 4 4 -2 -2 1 -1 3 -2 -1 3 3 5 * 12 8 1 6 1

14 2 0 1 2 -2 1 -5 1 -7 1 -4 3 12 * 12 5 3 -6

15 1 -1 -6 -4 1 4 2 1 0 1 0 4 8 12 * 11 3 1

16 3 1 -2 -1 1 -1 -1 -1 1 -2 -1 -2 1 5 11 * 19 7

17 3 2 -2 0 2 0 1 -1 2 2 0 0 6 3 3 19 * 16

18 -4 4 2 -2 4 2 4 4 0 0 0 -1 1 -6 1 7 16 *

Estimated Mean Multiplicities

3,2,1;1250

4.0

iN

NNm

i

idouble

ii

Section1 Section2 Section3 NM median

ANM 1.43±0.008 1.425±0.008 1.42±0.009 1.425

NANM 1.44±0.013 1.43±0.012 1.42±0.012 1.43

The dependence of mean multiplicity on the cutoff rigidity (measurements by ship borne 3NM-64 of IQSY

type in December 1966 – April 1967, Kodama & Ishida, 1967). By open circles are denoted mean multiplicities

of the ArNM and NANM

Mean Multiplicity and EAS

Average number of > 4σ spikes: 4±2Expected Number of > 4σ spikes according to gaussian( ) distribution: 0.126.1/2 ndf

)(***0

E

dEEASTN

GevE 60 10*3

A.Chilingarian G. Hovsepyan, E. Mamidjanyan, Study of Extensive Air Showers and Primary Energy Spectra by MAKET-ANI Detector on Mountain Aragats, Astroparticle Physics, 28 , pp 58-71, 2007.

Cross Sections of Photonuclear Reactions with air

Cross Section of Photo Nuclear Reaction of Photons with Nitrogen(continuous line) and Carbon(dotted line) Nucleus

Cross Section of Photo Nuclear Reaction of Photons with Oxygen Nuclei

Distribution of Mean Multiplicities of ARNM During Thunderstorm Activity

Multiplicity, m 1 2 3 4 5 6Nucleon Energy (Gev) NM64 0.07 0.12 0.18 0.25 0.4 0.64

C.J. Hatton, The Neutron Monitor, in J., G. Wilson and S.A. Wouthuysen (eds.), Progress in Elementary Particle and Cosmic-ray Physics, vol. 10, chapter 1, North Holland Publishing Co., Amsterdam, 1971

ConclusionsThe notion of the multiplicity, introduced several decades ago, despite its elegance did not become yet a basis of the physical analysis of any importance in the cosmic ray physics and space weather research. Here we introduce method of calculation of the mean multiplicity and demonstrate its relation to the high energy primary cosmic ray physics and to new observed high energy phenomena in the thunderstorm atmospheres. We demonstrate the “bursts” in the mean multiplicity time series measured by Aragats Neutron Monitor are connected with the incident Extensive Air Shower initiated by the primary particles with energies greater than 1 PeV and by the low energy neutron photo production by the gamma rays from the RREA process.