Instantaneous phase and amplitude correlation in the solar cycle
In the present study we address the issue of discerning between deterministic and stochastic paradigms in order to understand the behavior of the solar cycle. To this end we show the degree of correlation between the instantaneous amplitude and frequency in the sunspot number time series by the use...
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2002
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| LEADER | 06591caa a22008057a 4500 | ||
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| 001 | PAPER-5150 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518203446.0 | ||
| 008 | 190411s2002 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0036061323 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Mininni, P.D. | |
| 245 | 1 | 0 | |a Instantaneous phase and amplitude correlation in the solar cycle |
| 260 | |c 2002 | ||
| 270 | 1 | 0 | |m Mininni, P.D.; Departamento de Física, Fac. de Ciencias Exactas y Naturales, Universidad de Buenos Aires, C. Universitaria, 1428 Buenos Aires, Argentina |
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a In the present study we address the issue of discerning between deterministic and stochastic paradigms in order to understand the behavior of the solar cycle. To this end we show the degree of correlation between the instantaneous amplitude and frequency in the sunspot number time series by the use of the Gabor analytic signal. We compare this correlation with those arising from two theoretical models: (a) the Barnes model of widespread use in the literature and (b) a spatial truncation of the MHD equations. We show that comparisons between the correlation observed in the sunspot time series with those arising from theoretical models can be used to refute one of the models. |l eng | |
| 536 | |a Detalles de la financiación: Universidad de Buenos Aires, X209/00 | ||
| 536 | |a Detalles de la financiación: Fundación Antorchas | ||
| 536 | |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas, PIP02693/00 | ||
| 536 | |a Detalles de la financiación: We would like to thank for very fruitful comments made by an anonymous referee, which contributed to improving the present manuscript. This research was supported by the University of Buenos Aires (grant X209/00). The authors also acknowledge partial support from Fundación Antorchas and CONICET (grant PIP02693/00). | ||
| 593 | |a Departamento de Física, Fac. de Ciencias Exactas y Naturales, Universidad de Buenos Aires, C. Universitaria, 1428 Buenos Aires, Argentina | ||
| 593 | |a Inst. Astro./Fis. Espacio (CONICET), C. Universitaria, 1428 Buenos Aires, Argentina | ||
| 700 | 1 | |a Gomez, D.O. | |
| 700 | 1 | |a Mindlin, G.B. | |
| 773 | 0 | |d 2002 |g v. 208 |h pp. 167-179 |k n. 1 |p Sol. Phys. |x 00380938 |w (AR-BaUEN)CENRE-2238 |t Solar Physics | |
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| 856 | 4 | 0 | |u https://doi.org/10.1023/A:1019658530185 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00380938_v208_n1_p167_Mininni |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v208_n1_p167_Mininni |y Registro en la Biblioteca Digital |
| 961 | |a paper_00380938_v208_n1_p167_Mininni |b paper |c PE | ||
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