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Registration of the KeV and MeV neutron burst associated with thunderstorms or lightning. Ashot Chilingaryan and Nikolay Bostanjyan A. Alikhanyan National Laboratory, Armenia. - PowerPoint PPT Presentation
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Registration of the KeV and MeV neutron burst associated with thunderstorms or
lightning
Ashot Chilingaryan and Nikolay Bostanjyan
A. Alikhanyan National Laboratory, Armenia
The measurements have been conducted by standard neutron monitor, sensitive to high
energy atmospheric neutrons and by moderator and lead free proportional counter.
Table1. Characteristics of an observed neutrons bursts associated with lightnings. Results have been obtained for the peaks (one-minute streams)
D/ M /Y (Nmax – Naverg )/18
on output 0.4 µs
(m^2/min)
(Nmax - Naverg ) /18
on output 1250 µs
(m^2/min)
Duration of events
(min)
Comments
08/05/09 72..3 ±1.8% 44..9±1.2% 2
21/05/09 * 83.3 ±1.8% 53.7±1.2% 9
21/05/09 93.7 ±1.8% 86.7±1.2% 9
26/05/09 51..9 ±1.8% 37.1±1.2% 2
03/06/09 90.3±1.8% 58.6±1.2% 4
08/07/09 63.7±1.8% 55.7±1.2% 19
09/07/09 72.4±1.8% 54.4±1.2% 4
20/08/09 ** 49.3±1.8% 37.6±1.2% 5
20/08/09 39.8±1.8% 30.9±1.2% 10
02/09/09 48..9±1.8% 34.5±1.2% 6
19/09/09 62.7±1.8% 45±1.2% 5
02/11/09 49.7±1.8% 34.5±1.2% 1
19/09/09 NA 430± 5% 21 σ - 8 Bare tube
26/08/10 NA 719 ± 1.8% 47σ 14.7±1.2 1.7 σ 2
Values of the excess neutrons associated with a lightning are presented. The black columns by Aragats neutron monitor, the red column by Nor Amberd NM. Both
devices are sensitive to MeV neutrons. The green column by “bare” tube (low-energy neutrons)
• In one case (red column) the excess neutrons ten times more others (black). They are neutrons MeV energies. They are much more of the neutrons of low energy. There can be such case?
050
100150200250300350400450500550600650700750
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15
Number of events
Nu
mb
er o
f ex
cess
neu
tro
ns
(m^
2/m
in
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15
On output 0.4mcs observed huge increase of the count rate of neutrons at 8:03 UT associated with lightning, but on 1250 mcs there is no increase of the
count of neutrons
26 August, 2010
-30369
121518212427303336394245
7:30 8:00 8:30 9:00 9:30 10:00 10:30 11:00 11:30 12:00
UT
Rel
ativ
e in
crea
se o
f n
eutr
ons
(%)
0
5
10
15
20
25
30
35
Sig
nal
fro
m p
osit
iv
Inte
rclo
ud
Lig
htn
ings
By NANM By Byurakan antenna
On 1250 mcs there is no increase of the count of neutrons at 8:03UT, but at 9:25, 10:20, 10 34, 10:40 and 11:04 increase of the neutrons are observed as during
0.4mcs
26 August, 2010
-3
-1.5
0
1.5
3
4.5
6
7.5
9
7:30 8:00 8:30 9:00 9:30 10:00 10:30 11:00 11:30
UT
Rel
ativ
e co
un
t ra
te o
f n
eutr
ons
(%)
0
5
10
15
20
25
30
Sig
nal
s fr
om p
ozit
iv
ligh
nin
gs (
clou
d-
grou
nd
)
by NANM 1250mcs by Byrakan antena
The neutron bursts registered on NM, have duration from one till 19 minutes that can mean neutrons are born not in the processes of a lightning, but in electric
fields of thunderstorms
0123456789
1011121314151617181920
1 2 3 4 5 6 7 8 9 10 11 12 13
Number of events
Du
rati
on
of
even
ts
(min
)
The high- energy neutrons (black points), do not show increase in the time when count rate of the low -energy neutrons sharply increases The number the excess
neutrons in peak equal 428n/min. N(σ) =21
19 September, 2009
-2.5
0
2.5
5
7.5
10
12.5
15
8:00 8:30 9:00 9:30
UT
Rel
ati
ve
incr
ease
of
hig
h-e
ner
gy
neu
tro
ns
-20
5
30
55
80
105
Rel
ati
ve
incr
ease
of
low
-en
erg
y n
eutr
on
s
By NANM By Bare tube
А burst of neutrons coincided with a lightning.
19 September, 2009
-150
153045607590
105
8:00 8:15 8:30 8:45 9:00 9:15 9:30 9:45
UT
Rel
ati
ve
incr
ease
of
neu
tron
s (%
)
1400
1500
1600
1700
1800
1900
2000
Fre
qu
ency
By bare tube (Nor Amberd) By the Aragats antenna
Summary
• Our researches have shown, that during a thunderstorms neutrons from KeV to MeV energies are born
• Our researches have shown, that excess neutrons can be born in electric fields of thunderclouds and also during lightnings