Zobrazeno 1 - 10
of 22
pro vyhledávání: '"V. E. Chertoprud"'
Publikováno v:
Geomagnetism and Aeronomy. 56:585-591
The influence of the earthquake probability diurnal variation on specific features in the weekend effect in global seismic activity is revealed. The dependence of the global earthquake number on the local time and its possible relation to a quiet sol
Publikováno v:
Solar Physics. 289:2867-2878
The aim of this article is to investigate how the background magnetic field of the Sun behaves in different hemispheres. We used SOHO/MDI data obtained during a period of eight years from 2003 to 2011 to analyze the intensity distribution of the back
Autor:
V. N. Obridko, V. E. Chertoprud
Publikováno v:
Astronomy Reports. 56:146-152
SOHO-MDI daily magnetic field synoptic data (a 14-year series of daily maps of the solar magnetic field intensity B available at the site http://soi.stanford.edu/magnetic/index5.html) have been used to analyze the dynamics of the photospheric magneti
Publikováno v:
Solar Physics. 272:59-71
A new coordinate system – heliomagnetic reference frame – has been proposed in which the great circle passes through the solar pole and the north pole of the magnetic dipole is considered as the central meridian. It is shown that, in the new coor
Autor:
V. E. Chertoprud, V. N. Obridko
Publikováno v:
Astronomy Letters. 37:358-366
SOHO/MDI magnetograms have been used to analyze the longitude distribution of the squared solar magnetic field 〈B2〉 in the activity cycle no. 23. The energy of the magnetic field (〈B2〉) is shown to change with longitude. However, these variat
Autor:
G. S. Ivanov-Kholodny, E. E. Goncharova, V. E. Chertoprud, L. N. Leshchenko, G. V. Givishvili
Publikováno v:
Geomagnetism and Aeronomy. 49:503-509
The 40-year period of observations of short-term variations (with characteristic times of up to 1–2 days) in the critical frequency of the ionospheric F2 layer (foF2) is analyzed. The continuous (with a step of 1 h) series of fluctuations (F) of th
Publikováno v:
Astronomy Letters. 35:424-431
Based on SOHO/MDI data (an archive of magnetic maps with a resolution of ∼2″), we have investigated the dynamics of the small-scale background magnetic field on the Sun in solar cycle 23. The cyclic variations and surface structure of the backgro
Publikováno v:
Astronomy Letters. 33:844-847
The small-scale (∼10″) stochastic properties of the solar magnetic field B are analyzed in terms of the two-dimensional model of a fractal Brownian process (the mean square of the difference between the field strengths at two points separated by
Publikováno v:
Geomagnetism and Aeronomy. 47:803-809
Based on the Nimbus-7 (1978–1992) data and the parameters of solar activity (Wolf numbers W, solar radioemission F 10.7) and the ionosphere (f 2 index of the critical frequency of the ionospheric F 2 layer normalized to noon), the fractal dimension
Publikováno v:
Coronal Magnetometry ISBN: 9781493920372
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dde99fd8de0c84ecdbd355345bae7247
https://doi.org/10.1007/978-1-4939-2038-9_15
https://doi.org/10.1007/978-1-4939-2038-9_15