Noise in wireless systems from solar radio bursts
Document Type
Article
Publication Date
1-1-2005
Abstract
Solar radio bursts were first discovered as result of their interference in early defensive radar systems during the Second World War (1942). Such bursts can still affect radar systems, as well as new wireless technologies. We have investigated a forty-year record of solar radio burst data (1960-1999) as well as several individual radio events in the 23rd solar cycle. This paper reviews the results of a portion of this research. Statistically, for frequencies f ∼ 1 GHz (near current wireless bands), there can be a burst with amplitudes >10 3 solar flux units (SFU; 1 SFU = 10 -22 W/m 2 ) every few days during solar maximum conditions, and such burst levels can produce problems in contemporary wireless systems. © 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
Identifier
28044459875 (Scopus)
Publication Title
Advances in Space Research
External Full Text Location
https://doi.org/10.1016/j.asr.2004.04.013
ISSN
02731177
First Page
2253
Last Page
2257
Issue
12
Volume
36
Grant
ATM-0077273
Fund Ref
National Science Foundation
Recommended Citation
Lanzerotti, L. J.; Gary, D. E.; Nita, G. M.; Thomson, D. J.; and MacLennan, C. G., "Noise in wireless systems from solar radio bursts" (2005). Faculty Publications. 19926.
https://digitalcommons.njit.edu/fac_pubs/19926
