Fourier Power Spectra of Solar Noise Storms

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00498335" target="_blank" >RIV/67985815:_____/18:00498335 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11207-018-1367-5" target="_blank" >http://dx.doi.org/10.1007/s11207-018-1367-5</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-018-1367-5" target="_blank" >10.1007/s11207-018-1367-5</a>

Result language
angličtina
Original language name
Fourier Power Spectra of Solar Noise Storms
Original language description
We analyzed three noise storms recorded on 200-400MHz Trieste Callisto radio spectra on 2 July 2012, 8 July 2012, and 16 July 2012 by the Fourier method. We divided intervals of the noise storms into five-minute intervals, and in these intervals we computed the mean Fourier spectra as a function of the wave numbers in the frequency and height-scale spaces. We found that these Fourier spectra, where the spectrum from the quiet-activity interval was subtracted, are power-law spectra.
Czech name
—
Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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