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Hα Line Polarization in the 2B/X4.8 Flare of 2002 July 23
作者单位:Zhi Xu,Qing-Rong Chen,Cheng Fang(Department of Astronomy, Nanjing University, Nanjing 210093);N.M.Firstova(Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, Siberian Division, Russia) 
基金项目:国家自然科学基金,Russian Foundation for Basic Research,国家自然科学基金,NKBRSFG 
摘    要:On 2002 July23,a 2B/X4.8 flare was observed in the Hα line spec-tropolarimetrically by the Large Solar Vacuum Telescope of Baikal Astrophysical Observatory.Linear polarization of 3%-10% was detected in the Hα line,particu-larly where the line showed central reversal.The linear polarization is mainly radial on the solar disk and appears at the impulsive phase of the hard X-ray and γ-ray bursts.It is limited to some relatively small regions of the flare.The polarization in a limited small region(~4″-5″)changed its direction within a short period of time(~10s).

关 键 词:天体物理观测  线性偏振作用  太阳观测  脉冲波  耀斑

Hα Line Polarization in the 2B/X4.8 Flare of 2002 July 23
Zhi Xu,N.M.Firstova,Qing-Rong Chen,Cheng Fang. Hα Line Polarization in the 2B/X4.8 Flare of 2002 July 23[J]. Chinese Journal of Astronomy and Astrophysics, 2003, 3(3): 266-276
Authors:Zhi Xu  N.M.Firstova  Qing-Rong Chen  Cheng Fang
Affiliation:[1]DepartmentofAstronomy,NanjingUniversity,Nanjing210093 [2]InstituteofSolar-TerrestrialPhysics,RussianAcademyofSciences,SiberianDivision,Russia
Abstract:
Keywords:Polarization-line: profile-Sun: flare
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