Zobrazeno 1 - 8
of 8
pro vyhledávání: '"V. V. Kasinsky"'
Publikováno v:
Advances in Geosciences, Vol 14, Pp 271-275 (2008)
Eruptive activity of the Sun produces a chain of extreme geophysical events: high-speed solar wind, magnetic field disturbances in the interplanetary space and in the geomagnetic field and also intense fluxes of energetic particles. Space storms can
Externí odkaz:
https://doaj.org/article/3dda6d1c665a42fba1878b56f1c7ef4f
Publikováno v:
Advances in Geosciences, Vol 14, Pp 271-275 (2008)
Advances in Geosciences
Advances in Geosciences, European Geosciences Union, 2008, 14, pp.271-275
Advances in Geosciences
Advances in Geosciences, European Geosciences Union, 2008, 14, pp.271-275
Eruptive activity of the Sun produces a chain of extreme geophysical events: high-speed solar wind, magnetic field disturbances in the interplanetary space and in the geomagnetic field and also intense fluxes of energetic particles. Space storms can
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a47e7ac9f9cfa7e3c26fd8cc46d72e48
https://www.adv-geosci.net/14/271/2008/
https://www.adv-geosci.net/14/271/2008/
Autor:
V. V. Kasinsky, R. T. Sotnicova
Publikováno v:
Astronomical & Astrophysical Transactions. 22:325-333
The flare energy distribution of ultraviolet Ceti-type stars has a power-law spectrum $N \propto E^{-b}$ . Solar optical flares have an identical power energy spectrum with $b \approx 0.80$ . In a ...
Autor:
V. V. Kasinsky
Publikováno v:
Astronomical & Astrophysical Transactions. 17:341-350
Data on the location of flares covering solar cycles 17–20 were used to construct vector R(ϕ, t) diagrams for the mean position of the flare scattering centre in the coordinate system of the sunspot centre. The R(ϕ, t)-diagram reveals a spatial a
Autor:
R. T. Sotnikov, V. V. Kasinsky
Publikováno v:
Astronomical & Astrophysical Transactions. 12:313-314
Energy distribution in solar flares and in UV Ceti stellar flares are similar and can be approximated by a power law. The value of the flare energy spectrum power law exponent is 0.47 < β < 0.93. It changes cyclically and correlates with Zurich Wolf
Autor:
R. T. Sotnikova, V. V. Kasinsky
Publikováno v:
Radiophysics and Quantum Electronics. 39:815-816
We present the results of the processing of flare location data in the coordinate system of bipolar spot groups rotating with proper angular velocity ω(ϕ) in 20 active regions (AR). The polar diagrams R=R(ψ) show the spatial modulation of flares w
Autor:
V. V. Kasinsky, R. T. Sotnikova
Publikováno v:
International Astronomical Union Colloquium. 104:255-258
Based on X-ray (1-8 Å) flux data for 1977-1987, the integral spectra of solar flare energy were computed. The energy spectra were approximated by a power law N(E) α; E~n, with N being the number of flares with energy in excess of E. It is shown tha
Autor:
V. V. Kasinsky
Publikováno v:
Symposium - International Astronomical Union. 43:432-434
In this paper common regularities in flare positions have been studied in relation to spots as the extreme points of the magnetic field. The angular distribution diagrams of flares reveal that equatorial-western shifts of flares occurred during the I