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Long-period variations in the magnetic field of small-scale solar structures
Tekijät: P. V. Strekalova, Yu. A. Nagovitsyn, A. Riehokainen, V. V. Smirnova
Kustantaja: MAIK NAUKA/INTERPERIODICA/SPRINGER
Julkaisuvuosi: 2016
Journal: Geomagnetism and Aeronomy
Tietokannassa oleva lehden nimi: GEOMAGNETISM AND AERONOMY
Lehden akronyymi: GEOMAGN AERONOMY+
Vuosikerta: 56
Numero: 8
Aloitussivu: 1052
Lopetussivu: 1059
Sivujen määrä: 8
ISSN: 0016-7932
DOI: https://doi.org/10.1134/S0016793216080211(external)
Tiivistelmä
Thirty small-scale structures in the solar atmosphere, i.e., facula nodes at +/-(20A degrees-46A degrees) latitudes, have been studied in order to analyze quasi-periodic variations in the magnetic field. SDO/HMI magnetograms have been used for this purpose. Long-period variations in the magnetic field strength of the considered objects in the 60-280 min range have been revealed as a result of data processing. It has been shown that there are no dependences between the magnetic field and period, nor between the magnetic field and object area. It has been assumed that the discovered variations are not natural oscillations of the magnetic field strength.
Thirty small-scale structures in the solar atmosphere, i.e., facula nodes at +/-(20A degrees-46A degrees) latitudes, have been studied in order to analyze quasi-periodic variations in the magnetic field. SDO/HMI magnetograms have been used for this purpose. Long-period variations in the magnetic field strength of the considered objects in the 60-280 min range have been revealed as a result of data processing. It has been shown that there are no dependences between the magnetic field and period, nor between the magnetic field and object area. It has been assumed that the discovered variations are not natural oscillations of the magnetic field strength.
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