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magnetic field changes associated with three successive M-class solar flares on 2002 July 26

Research in Astronomy and Astrophysics 2011年第6期11卷 692-700页

作者： Pu Wang Ming-De Ding Hai-Sheng Ji Hai-Min Wang epartment of Astronomy Nanjing UniversityNanjing 210093China Purple Mountain Observatory Chinese Academy of SciencesNanjing 210008China Space Weather Research Lab Center for Solar Terrestrial ResearchNew Jersey Institute of TechnologyNewarkNJ 07102US

With an extensive analysis,we study the temporal evolution of magnetic flux during three successive M-class flares in two adjacent active regions：NOAA 10039 and *** primary data are full disk longitudinal magnetograms observed by SOHO/*** three flares are observed to be accompanied by magnetic flux *** changes occurred immediately or within 1 ～ 10 minutes after the starting time of the flares,indicating that the changes are obvious consequences of the solar *** changes in many points are intrinsic in magnetic flux,for some sites,it is caused by a rapid expansion motion of magnetic *** the second flare,the associated change is more gradual compared with the ＇step-function＇ reported in ***,we use the data observed by the Imaging Vector Magnetograph（IVM） at Mees Solar Observatory to check possible line profile changes during the *** results from the IVM data confirm the flux changes obtained from the MDI data.A series of line profiles were obtained from the IVM＇s observations and analyzed for flux change *** find that the fluctuations in the width,depth and central wavelength of the lines are less than 5.0 even at the flare＇s *** line profile change is observed during or after the *** conclude that the magnetic field changes associated with the three solar flares are not caused by flare emission.

关键词： sun:activity-sun:magnetic field-sun:flares

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