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Multiscale Comparative Spectral Analysis of Satellite Total Solar Irradiance Measurements from 2003 to 2013 Reveals a Planetary Modulation of Solar Activity and Its Nonlinear Dependence on the 11 Yr Solar Cycle : Volume 1, Issue 1 (25/11/2013)

By Scafetta, N.

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Book Id: WPLBN0004021455
Format Type: PDF Article :
File Size: Pages 11
Reproduction Date: 2015

Title: Multiscale Comparative Spectral Analysis of Satellite Total Solar Irradiance Measurements from 2003 to 2013 Reveals a Planetary Modulation of Solar Activity and Its Nonlinear Dependence on the 11 Yr Solar Cycle : Volume 1, Issue 1 (25/11/2013)  
Author: Scafetta, N.
Volume: Vol. 1, Issue 1
Language: English
Subject: Science, Pattern, Recognition
Collections: Periodicals: Journal and Magazine Collection, Copernicus GmbH
Historic
Publication Date:
2013
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

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Scafetta, N., & Willson, R. C. (2013). Multiscale Comparative Spectral Analysis of Satellite Total Solar Irradiance Measurements from 2003 to 2013 Reveals a Planetary Modulation of Solar Activity and Its Nonlinear Dependence on the 11 Yr Solar Cycle : Volume 1, Issue 1 (25/11/2013). Retrieved from http://www.ebooklibrary.org/


Description
Description: Active Cavity Radiometer Irradiance Monitor (ACRIM) Lab, Coronado, CA 92118, USA. Herein we adopt a multiscale dynamical spectral analysis technique to compare and study the dynamical evolution of the harmonic components of the overlapping ACRIMSAT/ACRIM3 (Active Cavity Radiometer Irradiance Monitor Satellite/Active Cavity Radiometer Irradiance Monitor 3), SOHO/VIRGO (Solar and Heliopheric Observatory/Variability of solar Irradiance and Gravity Oscillations), and SORCE/TIM (Solar Radiation and Climate Experiment/Total Irradiance Monitor) total solar irradiance (TSI) records during 2003.15 to 2013.16 in solar cycles 23 and 24. The three TSI time series present highly correlated patterns. Significant power spectral peaks are common to these records and are observed at the following periods: ~ 0.070 yr, ~ 0.097 yr, ~ 0.20 yr, ~ 0.25 yr, ~ 0.30–0.34 yr, and ~ 0.39 yr. Less certain spectral peaks occur at about 0.55 yr, 0.60–0.65 yr and 0.7–0.9 yr. Four main frequency periods at ~ 4.8 days (~ 0.068 yr), ~ 27.3 days (~ 0.075 yr), at ~ 34–35 days (~ 0.093–0.096 yr), and ~ 36–38 days (~ 0.099–0.104 yr) characterize the solar rotation cycle. The amplitude of these oscillations, in particular of those with periods larger than 0.5 yr, appears to be modulated by the ~ 11 yr solar cycle. Similar harmonics have been found in other solar indices. The observed periodicities are found highly coherent with the spring, orbital and synodic periods of Mercury, Venus, Earth and Jupiter. We conclude that solar activity is likely modulated by planetary gravitational and electromagnetic forces acting on the Sun. The strength of the Sun’s response to planetary forcing depends nonlinearly on the state of internal solar dynamics; planetary–Sun coupling effects are enhanced during solar activity maxima and attenuated during minima.

Summary
Multiscale comparative spectral analysis of satellite total solar irradiance measurements from 2003 to 2013 reveals a planetary modulation of solar activity and its nonlinear dependence on the 11 yr solar cycle

Excerpt
Abreu, J. A., Beer, J., Ferriz-Mas, A., McCracken, K. G., and Steinhilber, F.: Is there a planetary influence on solar activity?, Astron. Astrophys., 548, A88, doi:10.1051/0004-6361/201219997, 2012.; Brown, E. W.: A Possible Explanation of the Sun-spot Period, Mon. Not. R. Astron. Soc., 60, 599–606, 1900.; Bartels, J.: Twenty-seven day recurrences in terrestrial-magnetic and solar activity, 1923–1933, J. Geophys. Res., 39, 201–202a, doi:10.1029/TE039i003p00201, 1934.; Caballero, R. and Valdés-Galicia, J. F.: Statistical Analysis of the Fluctuations Detected in High-Altitude Neutron Monitor, Solar and Interplanetary Parameters, Sol. Phys., 213, 413–426, 2003.; Callebaut, D. K., de Jager, C., and Duhau, S.: The influence of planetary attractions on the solar tachocline, J. Atmos. Sol.-Terr. Phy., 80, 73–78, 2012.; Charbonneau, P.: Solar physics: The planetary hypothesis revived, Nature, 493, 613–614, 2013.; Charvátová, I.: Long-term predictive assessments of solar and geomagnetic activities made on the basis of the close similarity between the solar inertial motions in the intervals 1840–1905 and 1980–2045, New Astron., 14, 25–30, 2009.; Doodson, A. T.: The harmonic development of the tide-generating potential, P. Roy. Soc. Lond. A, 100, 305–329, 1921.; Fairbridge, R. W. and Shirley, J. H.: Prolonged minima and the 179-year cycle of the solar inertial motion, Sol. Phys., 10, 191–210, 1987.; Fröhlich, C.: Solar irradiance variability since 1978: revision of the PMOD composite during solar cycle 21, Space Sci. Rev., 125, 53–65, 2006.; Fröhlich, C.: Revised characterization of the PMO6V radiometers, ISSI, Bern, Switzerland, 14 May 2013.; Hung, C.-C.: Apparent Relations Between Solar Activity and Solar Tides Caused by the Planets, NASA/TM-2007-214817, 2007.; Jose, P. D.: Sun's motion and sunspots, Astron. J., 70, 193–200, 1965.; Kelvin (Lord, Thomson, W.): The tide gauge, tidal harmonic analyzer, and tide predictor, P. I. Civil Eng., 65, 3–24, 1881.; Kilcik, A., Özgüc, A., Rozelot, J. P., and Atas, T.: Periodicities in solar flare index for cycles 21–23 revisited, Solar Phys., 264, 255–268, 2010.; Kopp, G. and Lawrence, G.: The Total Irradiance Monitor (TIM): Instrument, Design, Sol. Phys., 230, 91–109, 2005.; Kopp, G., Heuerman, K., and Lawrence, G.: The Total Irradiance Monitor; (TIM): Instrument Calibration, Sol. Phys., 230, 111–127, 2005.; Pap, J., Tobiska, W. K., and Bouwer, S. D.: Periodicities of solar irradiance and solar activity indices, I., Sol. Phys., 129, 165–189, 1990.; Press, W. H., Teukolsky, S. A., Vetterling, W. T., and Flannery, B. P.: Numerical Recipes in C, 2nd Edn., Cambridge University Press, 1997.; Rieger, E., Kanbach, G., Reppin, C., Share, G. H., Forrest, D. J., and Chupp, E. L.: A 154-day periodicity in the occurrence of hard solar flares?, Nature, 312, 623–625, 1984.; Scafetta, N.: Empirical evidence for a celestial origin of the climate oscillations and its implications, J. Atmos. Sol.-Terr. Phy., 72, 951–970, doi:10.1016/j.jastp.2010.04.015, 2010a.; Scafetta, N.: Spectral analysis of the TSI satellite records, their comparison and interpretation. Abstract #GC21B-0868 (presented at 2010 Fall Meeting, AGU, San Francisco, Calif., 13–17 December 2010), 2010b.; Scafetta, N.: A shared frequency set between the historical mid-latitude aurora records and the global surface temperature, J. Atmos. Sol.-Terr. Phy., 74, 145–163, doi:10.1016/j.jastp.2011.10.013, 2012a.; Scafetta, N.: Testing an astronomically based decadal-scale empirical harmonic climate model versus the IPCC (2007) general circulation climate models, J. Atmos. Sol.-Terr. Phy., 80, 124–137,

 

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