Affiliation:
1. Главная астрономическая обсерватория РАН
2. Central Astronomical Observatory of Pulkovo of RAS
Abstract
This paper considers a longitude distribution of sunspot groups over 1982–2013, using data from the National Geophysical Data Center (Boulder, USA). The space-time distribution of sunspot groups is analyzed in coordinate sectors calculated from heliographic longitudes of the groups. A longitude extent of a coordinate sector is compared to the average size of one active region (30–40°). Then, in each coordinate sector, evolutionary activity of sunspot groups is summarized according to classification values after Malde throughout the observation period. The longitude distribution of large sunspot groups plotted in such a way does not reveal anticorrelation between Northern and Southern hemispheres in sunspot cycle 23.
Publisher
Infra-M Academic Publishing House
Subject
Space and Planetary Science,Atmospheric Science,Geophysics
Reference19 articles.
1. Astaf’eva N.M. Wavelet analysis: Theory grounds and examples of applications. Uspekhi fizicheskikh nauk. [Physics-Uspekhi (Advances in Physical Sciences)]. 1996, vol. 166, iss. 11, pp. 1145–1170. (In Russian)., Astaf’eva N.M. Wavelet analysis: Theory grounds and examples of applications. Uspekhi fizicheskikh nauk. [Physics-Uspekhi (Advances in Physical Sciences)]. 1996, vol. 166, iss. 11, pp. 1145–1170. (In Russian).
2. Benevolenskaya E.E., Hoeksema J.T., Kosovichev A.G., Scherrer P.H. The interaction of new and old magnetic fluxes at the beginning of solar cycle 23. The Astrophys. J. 1999, vol. 517, iss. 2, pp. 163–166. DOI: 10.1086/312046., Benevolenskaya E.E., Hoeksema J.T., Kosovichev A.G., Scherrer P.H. The interaction of new and old magnetic fluxes at the beginning of solar cycle 23. The Astrophys. J. 1999, vol. 517, iss. 2, pp. 163–166. DOI: 10.1086/312046.
3. Cowling T.G. On the Sun´s general magnetic field. Monthly Notices of the Royal Astronomical Society. 1945, vol. 105, p. 166. DOI: 10.1093/mnras/105.3.166., Cowling T.G. On the Sun´s general magnetic field. Monthly Notices of the Royal Astronomical Society. 1945, vol. 105, p. 166. DOI: 10.1093/mnras/105.3.166.
4. Erofeev D.V. The relationship between kinematics and spatial structure of the large-scale solar magnetic field. Solar Phys. 1997, vol. 175, iss. 1, pp. 45–58. DOI: 10.1023/ A:1004981317538., Erofeev D.V. The relationship between kinematics and spatial structure of the large-scale solar magnetic field. Solar Phys. 1997, vol. 175, iss. 1, pp. 45–58. DOI: 10.1023/ A:1004981317538.
5. Ivanov E.V. On space-time distribution of faculae and sunspots. Solnechnye dannye. Byul. [Solar Data Bulletin] 1986, no. 7, p. 61. (In Russian)., Ivanov E.V. On space-time distribution of faculae and sunspots. Solnechnye dannye. Byul. [Solar Data Bulletin] 1986, no. 7, p. 61. (In Russian).
Cited by
1 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Prototype solar dome designed to function as a solar calendar;Journal of Asian Architecture and Building Engineering;2024-07-02