Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-26T18:57:41.031Z Has data issue: false hasContentIssue false
  • English
  • Français

Sun-planets tidal interactions: an extended catalog

Published online by Cambridge University Press:  16 October 2024

Sergey M. Kudryavtsev Open the ORCID record for Sergey M. Kudryavtsev [Opens in a new window] ,
Rodolfo G. Cionco  and
Willie W.-H. Soon
Sergey M. Kudryavtsev*
Affiliation:
M.V. Lomonosov Moscow State University, Sternberg Astronomical Institute, 13, Universitetsky Pr., Moscow, Russia
Rodolfo G. Cionco
Affiliation:
CONICET and Grupo de Estudios Ambientales UTN, Colón 332, San Nicolás, Buenos Aires, Argentina
Willie W.-H. Soon
Affiliation:
Center for Environmental Research and Earth Sciences (CERES), Salem, MA 01970, USA Institute of Earth Physics and Space Science (ELKH EPSS), H-9400, Sopron, Hungary
*
email: ksm@sai.msu.ru
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An extended catalog of long-periodic terms of the Sun tide-generating potential (STGP ver.2) is released. It contains 2.5 times of such terms than in the first version of the STGP catalog (Cionco et al. 2023). The analysis of the new data is done in order to re-examine the existence of tidal forces of ≈ 11.0-yr and ≈ 22.0-yr period able to excite the observed solar-activity cycles. In several recent studies, such tidal forcings are claimed to be a result of certain combinations of Venus, Earth and Jupiter mean motions with the multipliers (6, −10, 4) and (3, −5, 2), respectively. So, in this contribution, we specifically look for the periodic terms related to these combinations. As a result of these additional investigation we do not confirm any noticeable tidal forcing factors of ≈ 11.0-yr nor ≈ 22.0-yr period in the extended STGP spectrum either.

Keywords

Solar CycleModelsOscillationsEphemerides
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S382: Complex Planetary Systems II: Latest Methods for an Interdisciplinary Approach , December 2022 , pp. 139 - 141
Check for updates
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Archinal, B. A., Acton, C. H., A’Hearn, M. F., et al. 2018, Celest. Mech. Dyn. Astron., 130, 22 CrossRefGoogle Scholar
Cionco, R. G., Kudryavtsev, S. M., Soon, W. W.-H. 2021, Earth and Space Sci., 8, e2021EA001805CrossRefGoogle Scholar
Cionco, R. G., Kudryavtsev, S. M., Soon, W. W.-H. 2023, Sol. Phys., 298:70 CrossRefGoogle Scholar
Kudryavtsev, S. M. 2004, J. Geodesy, 77, 829 CrossRefGoogle Scholar
Kudryavtsev, S. M. 2007, A&A, 471, 1069 Google Scholar
Kudryavtsev, S. M. 2016, MNRAS, 456, 4015 CrossRefGoogle Scholar
Kudryavtsev, S. M. 2017, MNRAS, 466, 2675 CrossRefGoogle Scholar
Kudryavtsev, S. M., Kudryavtseva, N. S. 2009, Celest. Mech. Dyn. Astron., 105, 353 CrossRefGoogle Scholar
Park, R. S., Folkner, W. M., Williams, J. G., Boggs, D. H. 2021, AJ, 161:105 CrossRefGoogle Scholar
Simon, J.-L., Bretagnon, P., Chapront, J., et al. 1994, A&A, 282, 663 Google Scholar
Stefani, F., Horstmann, G.M., Klevs, M., et al. 2023, arXiv:2309.00666v2Google Scholar
Supplementary material: PDF

Kudryavtsev et al. supplementary material

Kudryavtsev et al. supplementary material

Download Kudryavtsev et al. supplementary material(PDF)
PDF 1 MB