On the nature of the steep changes in solar and geomagnetic activity after 1705, 1923 and 1993
It was shown that the 11-year cycle amplitude modulation has suffered an ascending chaotic transition after 1923, leading the solar mean magnetic field almost to duplicate in less than 30 years, and that a descending transition started at year 1993.To investigate the nature of these steep changes we...
Guardado en:
| Autor principal: | |
|---|---|
| Formato: | Acta de conferencia Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2003
|
| Acceso en línea: | Registro en Scopus Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 05015caa a22004937a 4500 | ||
|---|---|---|---|
| 001 | PAPER-4810 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250228081850.0 | ||
| 008 | 190411s2003 xx ||||fo|||| 10| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0141939636 | |
| 030 | |a ESPUD | ||
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Duhau, Silvia Noemí Catalina | |
| 245 | 1 | 3 | |a On the nature of the steep changes in solar and geomagnetic activity after 1705, 1923 and 1993 |
| 260 | |c 2003 | ||
| 270 | 1 | 0 | |m Duhau, S.; Departamento de Fisica, Fac. de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina; email: duhau@df.uba.ar |
| 504 | |a Feyman, Gabriel, Period and phase of the 88-year Solar Cycle (1990) Solar Phys., 127, pp. 393-403 | ||
| 504 | |a Duhau, S., Chen, The sudden increases of Solar and Geomagnetic Activity after 1923 as a manifesta tion of a non-linear solar dynamo (2002) Geophys. Res. Lett, 13, pp. 6-1 | ||
| 504 | |a Duhau, S., An Early Prediction of Maximum Sunspot Cycle 24 (2003) Solar Phys., 213, pp. 203-212 | ||
| 504 | |a Duhau, S., Two coupled 88 and 22 yr. oscillators in the Modulation of Sunspot cycle (2002) Anales AFA, 13, p. 37 | ||
| 504 | |a Duhau, S., Chen, C., A multi resolution analysis of the relationship between the solar sunspot number and the geomagnetic index aa (2000) Anales AFA, 11, p. 326 | ||
| 504 | |a Mayaud, P.N., Analysis of Sudden Commencements for the Years 1868-1967 J. Geophys. Res., 80, pp. 111-122 | ||
| 504 | |a Oliver, R.J., Emergence of Magnetic Flux at the Sun as the Cause of a 158-day periodicity in Suspot Areas (1996) Nature, 163, pp. 552-553 | ||
| 504 | |a Silva, A., Duhau, S., Estudio de Periodicidades en la Tasa de Ocurrencia de Fulguraciones - Gamma y en Areas de Manchas Solares Durante la Misión CGRO Anales AFA, 14. , in revision | ||
| 504 | |a Ballester, J.L., (2000) Astrophys. J., 566, pp. 505-511 | ||
| 504 | |a Schmitt, D., Intermittent solar activity by an on-off dynamo (1996) Astron. Astrhophys., 311, pp. L1-L4 | ||
| 504 | |a Durney, (2000) Solar Phys., 196, pp. 421-439 | ||
| 504 | |a Boncho, B., Estimating the course of the solar activity in the end of the 20th Century and the beginning of the 21st Century on Time Variation within the Zurich Time Series (1997) Bulgarian Geophys. Journal, 43-48A4 - Scientific Committee on Solar-Terrestrial Physics (SCOSTEP); International Astronomical Union (IAU); European Space Agency (ESA); Committee on Space Research (COSPAR); U.S. National Science Foundation (NSF) | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a It was shown that the 11-year cycle amplitude modulation has suffered an ascending chaotic transition after 1923, leading the solar mean magnetic field almost to duplicate in less than 30 years, and that a descending transition started at year 1993.To investigate the nature of these steep changes we perform a multi-resolution wavelet analysis of the relationship between long term evolution in Wolf sunspot number, geomagnetic index aa time series and 158-day periodicity in sunspots (1844-2002). The same methodology is applied to the study of the sudden commencement index (SSC) (1968-1993), defined for each storm as the product of its amplitude and rise time.We find that the chaotic ascending transition is synchronic with the strengthening of the 158-day periodicity, while the SSC index is inversely related to the 158 days periodicity and had reached during sunspot cycle 22 its largest value since 1868.In the light of dynamo theory we conclude that new magnetic flux has been injected to the dynamo layer from the convective region during the ascending transition wile during cycle 22 strong toroidal fields were ejected by the solar dynamo system leading to intense sudden commencement geomagnetic storms. |l eng | |
| 593 | |a Departamento de Fisica, Fac. de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina | ||
| 690 | 1 | 0 | |a GEOMAGNETISM |
| 690 | 1 | 0 | |a MAGNETIC FIELDS |
| 690 | 1 | 0 | |a MAGNETIC FLUX |
| 690 | 1 | 0 | |a GEOMAGNETIC ACTIVITY |
| 690 | 1 | 0 | |a SOLAR ENERGY |
| 711 | 2 | |c Tatranska Lomnica |d 23 June 2003 through 28 June 2003 |g Código de la conferencia: 61608 | |
| 773 | 0 | |d 2003 |h pp. 91-94 |k n. 535 |p Eur Space Agency Spec Publ ESA SP |n European Space Agency, (Special Publication) ESA SP |x 03796566 |t Proceedings of the ISCS 2003; Solar Variability as an Input to the Earth's Environment | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-0141939636&partnerID=40&md5=2085577385525c52c4ed1bfc245b33a5 |y Registro en Scopus |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_03796566_v_n535_p91_Duhau |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n535_p91_Duhau |y Registro en la Biblioteca Digital |
| 961 | |a paper_03796566_v_n535_p91_Duhau |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/conferenceObject |a info:ar-repo/semantics/documento de conferencia |b info:eu-repo/semantics/publishedVersion | ||
| 999 | |c 65763 | ||