At Basic Environmental Observatory (BEO) Moussala (2925 m a.s.l.) and at Lomnický štít (LS) (2634 m a.s.l.) there are now working similar detector systems of the Space Environmental Viewing and Analysis Network (SEVAN) type. Using data from overlapping period (2014 - 2017) we estimate the barometric pressure coefficient for various channels of SEVANs and for various seasons. For thunderstorm periods the short time increases at SEVANs corresponding to the local high electric field, and most probably being the thunderstorm ground enhancements (TGE) events, are presented. Similarities and differences in the responses of SEVAN to thunderstorm events at the two sites are discussed. In what follows we examine the comprehensive meteorological data from the LS and BEO Moussala mountain observatories in comparison with Global data to answer the question: is there support for the hypothesis that CR contribute significantly to the local climate, by way of enhanced cloud cover?

Topics
Weather hazard, Network analysis, News and events
1.
A.
 
Chilingarian
,
T.
 
Karapetyan
,
Advances in Space Research
,
47
,
1140
–
1146
(
2011
).
https://doi.org/10.1016/j.asr.2010.12.001
Google Scholar
Crossref
Search ADS
 
2.
A.
 
Chilingarian
,
V.
 
Babayan
,
T.
 
Karapetyan
,
B.
 
Mailyan
,
B.
 
Sargsyan
,
M.
 
Zazyan
,
Advances in Space Research
,
61
,
2680
–
2696
(
2018
).
https://doi.org/10.1016/j.asr.2018.02.030
Google Scholar
Crossref
Search ADS
 
3.
A.
 
Chilingarian
,
G.
 
Hovsepyan
,
K.
 
Arakelyan
, et al. 
Earth, Moon, and Planets
 
104
,
195
–
210
(
2009
)
https://doi.org/10.1007/s11038-008-9288-1
.
Google Scholar
Crossref
Search ADS
 
4.
A.
 
Chilingarian
,
A.
 
Reymers
,
Annales Geophysicae
,
26
,
249
–
257
(
2008
).
https://doi.org/10.5194/angeo-26-249-2008
Google Scholar
Crossref
Search ADS
 
5.
K.
 
Kudela
,
J.
 
Chum
,
M.
 
Kollárik
,
R.
 
Langer
,
I.
 
Strhárský
,
J.
 
Baše
,
Correlations between secondary cosmic ray rates and strong electric fields at Lomnický štít
.
Journal of Geophysical Research: Atmospheres
,
122
,
10,700
–
10,710
 
https://doi.org/10.1002/2016JD026439
(
2017
).
Google Scholar
Crossref
Search ADS
 
6.
E.
 
Samara
,
A.
 
Smponias
,
I.
 
Lytrosyngounis
,
D.
 
Lingri
,
H.
 
Mavromichalaki
,
C. Sgouropoulos Solar Phys.
,
217
,
293
–
67
(
2018
).
Google Scholar
 
7.
De-Hong
 
Huang
,
Hong-Qiao
 
Hu
,
Ji-Long
 
Zhang
,
Hong
 
Lu
,
Da-Li
 
Zhang
,
Bin-Shen
 
Xue
,
Jing-Tian
 
Lu
, https://arxiv.org/ftp/arxiv/papers/1710/1710.00945.pdf (
2018
).
8.
A.
 
Tchorbadjiev
,
I.
 
Angelov
,
Ch.
 
Angelov
,
N.
 
Nikolova
,
T.
 
Arsov
,
I.
 
Kalapov
,
A.
 
Boyadjieva
,
Bulgarian Astronomical Journal
,
18
, (
2012
).
Google Scholar
 
9.
A.
 
Tchorbadjieff
,
Ch.
 
Angelov
,
I.
 
Angelov
,
T.
 
Arsov
,
I.
 
Kalapov
,
N.
 
Nikolova
,
A.
 
Boyadjieva
,
C. R. Acad. Bulg. Sci.
 
66
,
659
–
666
(
2013
).
Google Scholar
Crossref
Search ADS
 
10.
A.
 
Smponias
,
I.
 
Lytrosyngounis
,
E.
 
Samara
,
D.
 
Lingri
,
H.
 
Mavromichalaki
 http://www.stce.be/esww14/contributions/public/S10-P1/S10-P1-06-LingriDimitra/ESSW14_Smponiasetal_CRVARIATIONS.pdf (
2017
).
11.
J.
 
Guo
,
M.
 
Dumbović
,
R. F.
 
Wimmer-Schweingruber
,
M.
 
Temmer
,
H.
 
Lohf
,
Y.
 
Wang
,
A.
 
Veronig
,
D. M.
 
Hassler
,
L. M.
 
Mays
,
C.
 
Zeitlin
,
B.
 
Ehresmann
,
O.
 
Witasse
,
J. L. Freiherr
 
von Forstner
,
B.
 
Heber
,
M.
 
Holmström
,
Arik Posner
 https://arxiv.org/pdf/1803.00461.pdf (
2018
).
Google Scholar
 
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