The magnetic field reversal of the large-scale magneticfield was found as manifested in polarization of radio emission of the Sun dur-ing cycles of solar activity numbers 22-23. The analysis of polarization of radioemission for the structures of various brightness temperature has been carriedout. ...
We found polarization drifts of radio emission in the high-latitudes activity and at latitude band of the sunspots Process of the magnetic field reversal of the large-scale magnetic field in polarization of radio emission of the Sun was found during 22-23 cycles. An analysis of polarization for...
A study is performed of solar proton events that occurred during periods of the reversal of the Sun's magnetic field in cycles 19–24 of solar activity. Periods 8–12 months long and falling on the times of the magnetic field's reversal are found in each solar cycle. The number of ...
Geomagnetism & Aeronomy C/c of Geomagnetizm I AeronomiiaZolotova NV, Ponyavin DI (2013) Spatio-temporal sunspot impulses and reversal of the polar magnetic field on the sun. Ge &Ae 53: 945-948Zolotova NV, Ponyavin DI (2013) Spatio-temporal sunspot impulses and reversal of the polar ...
Konstantinova-Antova, A polarity reversal in the large-scale magnetic field of the rapidly rotating sun HD 190771. Astron. Astrophys. 508 , 9–12 (2009). : 10.1051/0004-6361/200913285 ADSPetit, P., Dintrans, B., Morgenthaler, A., Van Grootel, V., Morin, J., Lanoux, ...
Zolotova NV, Ponyavin DI (2013) Spatio-temporal sunspot impulses and reversal of the polar magnetic field on the sun. Ge & Ae 53:945-948Zolotova NV, Ponyavin DI (2013) Spatio-temporal sunspot impulses and reversal of the polar magnetic field on the sun. Ge & Ae 53:945–948...
The modulation consists of two discrete states (high and low intensities), corresponding respectively to those of the polarity of the polar magnetic field of the Sun. This can be interpreted on the basis of the following hypothesis; when the polar magnetic field of the Sun is nearly parallel ...
We were able to obtain a high (BH)max (1.6 MGOe) and thus take an important step in improving the magnetic properties of hard magnets without rare earth elements. 2. Experimental 2.1. Materials and Instrumentation In this study, the impact of adding different amounts of α-Fe on the ...
Sun X,Lin Y,Wang X.Reversal of magnetic field rota- tion in the reconnection layer due to shear flow effects. Journal of Geophysical Research . 2006Reversal of magnetic field rota- tion in the reconnection layer due to shear flow effects. Sun X,Lin Y,Wang X. Journal of Geophysical ...
The spatiotemporal organization of sunspots in the form of activity impulses (according to Gnevyshev's terminology) is considered as a source of poleward magnetic surges of new polarity. Polar fields in the northern and southern hemispheres have been reconstructed from 1875 to 2012. An increase ...