Zobrazeno 1 - 10
of 40
pro vyhledávání: '"A. F. Kharshiladze"'
Autor:
A. F. Kharshiladze, K. G. Ivanov
Publikováno v:
Geomagnetism and Aeronomy. 56:125-128
The results of a spherical harmonic analysis and a sector spherical harmonic analysis of the solar magnetic field on the photosphere, source surface, and in the Earth’s orbit on July 10–20, 2004, were compared. It was found that the field values
Autor:
R. A. Kislov, V. N. Obridko, A. F. Kharshiladze, Helmi Malova, Lev Zelenyi, Alessandro Bemporad, Olga Khabarova, V. D. Kuznetsov
An extensive analysis of Ulysses observations of the solar wind speed V from 1990 to 2008 is undertaken. It is shown that the evolution of V with heliocentric distance r depends substantially on both the heliolatitude and the solar activity cycle. De
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d82af8f614455736972e6eb4629c7b5f
Autor:
K. G. Ivanov, A. F. Kharshiladze
Publikováno v:
Geomagnetism and Aeronomy. 54:712-717
It was discovered that the dates of the earthquakes of the summer 2012, being ordered in accordance with the corresponding Carrington rotations (CR) of the Sun nos. 2123–2127, form four discrete isolated groups, with a 30-day periodicity of the ear
Autor:
A. F. Kharshiladze, K. G. Ivanov
Publikováno v:
Geomagnetism and Aeronomy. 54:537-548
The dynamics of solar-terrestrial relations in summer 2012 during passage from the growth phase to the maximum phase is considered. The four-sector structure of the Large-Scale Open Solar Magnetic Field (LOSMF) became more complicated because of a br
Autor:
K. G. Ivanov, A. F. Kharshiladze
Publikováno v:
Geomagnetism and Aeronomy. 53:677-689
The dynamics of the absolute global values (Φ) of the large-scale open solar magnetic field (LOSMF) fluxes at an interval of one solar rotation in 2006–2012 has been studied based on the Wilcox Solar Observatory data and using the ISOPAK original
Autor:
A. F. Kharshiladze, K. G. Ivanov
Publikováno v:
Geomagnetism and Aeronomy. 53:1-4
The theory of sector harmonic analysis has been developed as applied to the specific conditions of the solar magnetic field. A computer program has been developed. The possibilities of the program are illustrated in an analysis of a large-scale open
Autor:
K. G. Ivanov, A. F. Kharshiladze
Publikováno v:
Geomagnetism and Aeronomy. 52:1-15
We confirm the close synoptic relationship of the sectoral structure of the Sun’s magnetic field of the with the near-Earth tropospheric pressure with a case study of three European points (Troitsk, Rome, Jungfrau) in the period of the anomalously
Autor:
K. G. Ivanov, A. F. Kharshiladze
Publikováno v:
Geomagnetism and Aeronomy. 54:275-277
It has been shown that sector spherical harmonic analysis, in contrast to the usual harmonic analysis, allows for an exact coordination of the solar magnetic field from the photosphere to the Earth’s orbit.
Autor:
A. F. Kharshiladze, K. G. Ivanov
Publikováno v:
Geomagnetism and Aeronomy. 49:273-289
The MHD nature of the origination, dynamics, geoeffectiveness, and disappearance of the four-sector structure of the solar magnetic field during the cycle 23 decline phase has been established. A prolonged ordered MHD process including the chain of t
Autor:
A. F. Kharshiladze, K. G. Ivanov
Publikováno v:
Geomagnetism and Aeronomy. 48:578-594
The dynamics (from rotation to rotation) of the absolute values of the large-scale open solar magnetic field fluxes in the four-sector field structure has been considered for the first time, using CRs 2032–2035 in July–October 2005 as examples. A