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Titel |
On the scaling of the solar incident flux |
VerfasserIn |
C. A. Varotsos, S. Lovejoy, N. V. Sarlis, C. G. Tzanis, M. N. Efstathiou |
Medientyp |
Artikel
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Sprache |
Englisch
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ISSN |
1680-7316
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Digitales Dokument |
URL |
Erschienen |
In: Atmospheric Chemistry and Physics ; 15, no. 13 ; Nr. 15, no. 13 (2015-07-07), S.7301-7306 |
Datensatznummer |
250119872
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Publikation (Nr.) |
copernicus.org/acp-15-7301-2015.pdf |
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Zusammenfassung |
It was recently found that spectral solar incident flux (SIF) as
a function of the ultraviolet wavelengths exhibits 1/f-type
power-law correlations. In this study, an attempt was made to
explore the residues of the SIF with respect
to the Planck law over a wider range of wavelengths,
from 115.5 to 629.5 nm.
Using spectral, Haar and Detrended Fluctuation analyses, we show that over
the range from 10–20 nm to the maximum lag (≈ 500 nm), the SIF
residues have a scaling regime with fluctuation exponent H ≈ 0.37 but
with high intermittency (C1 ≈ 0.16, multifractal index
α≈ 1.7) and spectral exponent ≈ 1.46. Over the shorter
wavelengths range we found on the contrary low intermittency (C1 ≈ 0) with spectral exponent ≈ 1 and H ≈ 0. |
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