Dynamical characterization of the last prolonged solar minima
The planetary hypothesis of the solar cycle is an old idea in which the gravitational influence of the planets has a non-negligible effect on the causes of the solar magnetic cycle The advance of this hypothesis is based on phenomenological correlations between dynamical parameters of the Sun's...
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2012
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| LEADER | 15279caa a22013937a 4500 | ||
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| 005 | 20230518203903.0 | ||
| 008 | 190411s2012 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-84866740123 | |
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| 030 | |a ASRSD | ||
| 100 | 1 | |a Cionco, R.G. | |
| 245 | 1 | 0 | |a Dynamical characterization of the last prolonged solar minima |
| 260 | |c 2012 | ||
| 270 | 1 | 0 | |m Cionco, R.G.; Universidad Tecnológica Nacional (UTN), Facultad Regional San Nicolás, Colón 332, San Nicolás de los Arroyos 2900, Buenos Aires, Argentina; email: gcionco@frsn.utn.edu.ar |
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a The planetary hypothesis of the solar cycle is an old idea in which the gravitational influence of the planets has a non-negligible effect on the causes of the solar magnetic cycle The advance of this hypothesis is based on phenomenological correlations between dynamical parameters of the Sun's movement around the barycentre of the Solar System and sunspots time series; and more especially, identifying relationships linking solar barycentric dynamics with prolonged minima (especially Grand Minima events) However, at present there is no clear physical mechanism relating these phenomena The possible celestial influence on solar cycle modulation is of great importance not only in solar physics but also in Earth sciences, because prolonged solar minima have associated important climatic and telluric variations, in particular, during the Maunder and Dalton Minimum In this work we looked for a possible causal link in relation with solar barycentric dynamics and prolonged minima events We searched for particular changes in the Sun's acceleration and concentrated on long-term variations of the solar cycle We show how the orbital angular momentum of the Sun evolves and how the inclination of the solar barycentric orbit varies during the epochs of orbital retrogressions In particular, at these moments, the radial component of the Sun's acceleration (i.e.; in the barycentre-Sun direction) had an exceptional magnitude These radial impulses occurred at the very beginning of the Maunder Minimum, during the Dalton Minimum and also at the maximum of cycle 22 before the present extended minimum We also found a strong correlation between the planetary torque and the observed sunspots international number around that maximum We apply our results in a novel theory of Sun-planets interaction that it is sensitive to Sun barycentric dynamics and found a very important effect on the Sun's capability of storing hypothetical reservoirs of potential energy that could be released by internal flows and might be related to the solar cycle This process begins about 40 years before the solar angular momentum inversions, i.e.; before Maunder Minimum, Dalton Minimum, and before the present extended minimum Our conclusions suggest a dynamical characterization of peculiar prolonged solar minima We discuss the possible implications of these results for the solar cycle including the present extended minimum © 2012 COSPAR Published by Elsevier Ltd All rights reserved. |l eng | |
| 536 | |a Detalles de la financiación: PIP PIP 114-201001-00250 | ||
| 536 | |a Detalles de la financiación: ARC/11/09 | ||
| 536 | |a Detalles de la financiación: The authors are indebted to parallel processing facilities of Departamento de Ingeniería Mecánica de UTN-FRSN. The authors acknowledge the support of Grant PID-UTN 1351 “Forzantes externos al planeta y variabilidad climática” of UTN ; and Grant PICT – 2007 – 00438 of ANPCyT of Argentina. RHC is also supported by Grants UBACYT N°:20020100101049, CONICET PIP PIP 114-201001-00250, MINCYT-MEYS ARC/11/09. | ||
| 593 | |a Universidad Tecnológica Nacional (UTN), Facultad Regional San Nicolás, Colón 332, San Nicolás de los Arroyos 2900, Buenos Aires, Argentina | ||
| 593 | |a Universidad de Buenos Aires, Departamento de Ciencias de la Atmósfera y Los Océanos, Ciudad Universitaria, Pabellón II;CABA 1428, Argentina | ||
| 690 | 1 | 0 | |a GRAND MINIMA EVENTS |
| 690 | 1 | 0 | |a SOLAR ACTIVITY |
| 690 | 1 | 0 | |a SUN-EARTH CONNECTION |
| 690 | 1 | 0 | |a SUN-PLANETS INTERACTIONS |
| 690 | 1 | 0 | |a DYNAMICAL CHARACTERIZATION |
| 690 | 1 | 0 | |a DYNAMICAL PARAMETERS |
| 690 | 1 | 0 | |a GRAND MINIMA EVENTS |
| 690 | 1 | 0 | |a INTERNAL FLOWS |
| 690 | 1 | 0 | |a LONG-TERM VARIATIONS |
| 690 | 1 | 0 | |a MAUNDER MINIMUM |
| 690 | 1 | 0 | |a ORBITAL ANGULAR MOMENTUM |
| 690 | 1 | 0 | |a PHYSICAL MECHANISM |
| 690 | 1 | 0 | |a RADIAL COMPONENT |
| 690 | 1 | 0 | |a SOLAR ACTIVITY |
| 690 | 1 | 0 | |a SOLAR CYCLE |
| 690 | 1 | 0 | |a SOLAR CYCLE MODULATION |
| 690 | 1 | 0 | |a SOLAR MAGNETIC CYCLE |
| 690 | 1 | 0 | |a SOLAR MINIMA |
| 690 | 1 | 0 | |a SOLAR PHYSICS |
| 690 | 1 | 0 | |a STRONG CORRELATION |
| 690 | 1 | 0 | |a SUN-EARTH CONNECTION |
| 690 | 1 | 0 | |a ANGULAR MOMENTUM |
| 690 | 1 | 0 | |a DYNAMICS |
| 690 | 1 | 0 | |a PLANETS |
| 690 | 1 | 0 | |a SOLAR ENERGY |
| 690 | 1 | 0 | |a SUN |
| 700 | 1 | |a Compagnucci, R.H. | |
| 773 | 0 | |d 2012 |g v. 50 |h pp. 1434-1444 |k n. 10 |p Adv. Space Res. |x 02731177 |w (AR-BaUEN)CENRE-3577 |t Advances in Space Research | |
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