Computer Science
Scientific paper
Oct 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002kfnt...18..399l&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, vol. 18, no. 5, p. 399-409.
Computer Science
Scientific paper
We studied features of sector structures of the large-scale magnetic fields and their connection on the time scales corresponding to specific conditions of the solar activity (the cycle, the three-year intervals of different activity levels). For this purpose we performed a comparative analysis of power spectra of three time series 1976-1996: the intensity and sign of the overall magnetic field (OMF) of the Sun, as well as the sign of the interplanetary magnetic field (IMF). We concluded that the square of the magnetic structures, not the field intensity in their elements, is of crucial importance in forming and controlling of the sector structure of OMF and IMF. We derived that the two-sector and four-sector structures are independent phenomena of the solar magnetism and manifest themselves in different ways during the main phases of the cycles. The two-sector structure can be observed almost without exception and the four-sector one appears regularly every 8-9 years. We detected the change of two dominant rotational periods of the large-scale magnetic structures in antiphase during three-year time intervals.
No associations
LandOfFree
Variations of sector structures of the large-scale solar and interplanetary magnetic fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Variations of sector structures of the large-scale solar and interplanetary magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variations of sector structures of the large-scale solar and interplanetary magnetic fields will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1426590