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The influence of the solar flux at 2.8 GHz on outbreaks of gypsy moth (Lymantria dispar L.) (Lepidoptera: Lymantriidae) in Serbia

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2010
385.pdf (192.2Kb)
Authors
Milenković, M.
Ducić, Vladan
Milovanović, Boško
Article (Published version)
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Abstract
The connection between the solar flux at 2.8 GHz (based on mean monthly values) and the outbreaks of gypsy moths (Lymantria dispar L.) in Serbia was investigated. The researches included six outbreaks from 1952 to 2007. The average values of the solar flux ranged between 83.8 and 101.8 sfu during the outbreaks, whereas they were between 147.9 and 188.3 sfu for the periods without outbreaks. The results of the research showed that the increase in the number of gypsy moths appears when the values of the solar flux at 2.8 GHz range from 70 to 120 sfu.
Keywords:
gypsy moth / Lymantria dispar / outbreak / solar flux / solar activity / Serbia
Source:
Archives of Biological Sciences, 2010, 62, 4, 1021-1025
Publisher:
  • Srpsko biološko društvo, Beograd, i dr.

DOI: 10.2298/ABS1004021M

ISSN: 0354-4664

WoS: 000287217500019

Scopus: 2-s2.0-78650973908
[ Google Scholar ]
3
1
URI
https://gery.gef.bg.ac.rs/handle/123456789/387
Collections
  • Radovi istraživača
Institution/Community
Geografski fakultet
TY  - JOUR
AU  - Milenković, M.
AU  - Ducić, Vladan
AU  - Milovanović, Boško
PY  - 2010
UR  - https://gery.gef.bg.ac.rs/handle/123456789/387
AB  - The connection between the solar flux at 2.8 GHz (based on mean monthly values) and the outbreaks of gypsy moths (Lymantria dispar L.) in Serbia was investigated. The researches included six outbreaks from 1952 to 2007. The average values of the solar flux ranged between 83.8 and 101.8 sfu during the outbreaks, whereas they were between 147.9 and 188.3 sfu for the periods without outbreaks. The results of the research showed that the increase in the number of gypsy moths appears when the values of the solar flux at 2.8 GHz range from 70 to 120 sfu.
PB  - Srpsko biološko društvo, Beograd, i dr.
T2  - Archives of Biological Sciences
T1  - The influence of the solar flux at 2.8 GHz on outbreaks of gypsy moth (Lymantria dispar L.) (Lepidoptera: Lymantriidae) in Serbia
VL  - 62
IS  - 4
SP  - 1021
EP  - 1025
DO  - 10.2298/ABS1004021M
UR  - conv_577
ER  - 
@article{
author = "Milenković, M. and Ducić, Vladan and Milovanović, Boško",
year = "2010",
abstract = "The connection between the solar flux at 2.8 GHz (based on mean monthly values) and the outbreaks of gypsy moths (Lymantria dispar L.) in Serbia was investigated. The researches included six outbreaks from 1952 to 2007. The average values of the solar flux ranged between 83.8 and 101.8 sfu during the outbreaks, whereas they were between 147.9 and 188.3 sfu for the periods without outbreaks. The results of the research showed that the increase in the number of gypsy moths appears when the values of the solar flux at 2.8 GHz range from 70 to 120 sfu.",
publisher = "Srpsko biološko društvo, Beograd, i dr.",
journal = "Archives of Biological Sciences",
title = "The influence of the solar flux at 2.8 GHz on outbreaks of gypsy moth (Lymantria dispar L.) (Lepidoptera: Lymantriidae) in Serbia",
volume = "62",
number = "4",
pages = "1021-1025",
doi = "10.2298/ABS1004021M",
url = "conv_577"
}
Milenković, M., Ducić, V.,& Milovanović, B.. (2010). The influence of the solar flux at 2.8 GHz on outbreaks of gypsy moth (Lymantria dispar L.) (Lepidoptera: Lymantriidae) in Serbia. in Archives of Biological Sciences
Srpsko biološko društvo, Beograd, i dr.., 62(4), 1021-1025.
https://doi.org/10.2298/ABS1004021M
conv_577
Milenković M, Ducić V, Milovanović B. The influence of the solar flux at 2.8 GHz on outbreaks of gypsy moth (Lymantria dispar L.) (Lepidoptera: Lymantriidae) in Serbia. in Archives of Biological Sciences. 2010;62(4):1021-1025.
doi:10.2298/ABS1004021M
conv_577 .
Milenković, M., Ducić, Vladan, Milovanović, Boško, "The influence of the solar flux at 2.8 GHz on outbreaks of gypsy moth (Lymantria dispar L.) (Lepidoptera: Lymantriidae) in Serbia" in Archives of Biological Sciences, 62, no. 4 (2010):1021-1025,
https://doi.org/10.2298/ABS1004021M .,
conv_577 .

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