AR5395:OBSERVATIONS ON THE ASYMMETRIES OF THE Hα AND CaⅡ K LINE PROFILES OF THE FLARES ON MARCH 9 AND 14,1989

Fang Cheng; Hu Ju; Ji Guoping; Yin Suying; Zhang Qizhou

Fang Cheng, Hu Ju, Ji Guoping, Yin Suying, Zhang Qizhou. AR5395:OBSERVATIONS ON THE ASYMMETRIES OF THE Hα AND CaⅡ K LINE PROFILES OF THE FLARES ON MARCH 9 AND 14,1989[J]. Publications of the Yunnan Observatory, 1990, (4): 38-41.

Citation:

Fang Cheng, Hu Ju, Ji Guoping, Yin Suying, Zhang Qizhou. AR5395:OBSERVATIONS ON THE ASYMMETRIES OF THE Hα AND CaⅡ K LINE PROFILES OF THE FLARES ON MARCH 9 AND 14,1989[J]. Publications of the Yunnan Observatory, 1990, (4): 38-41.

Citation:

Fang Cheng, Hu Ju, Ji Guoping, Yin Suying, Zhang Qizhou. AR5395:OBSERVATIONS ON THE ASYMMETRIES OF THE Hα AND CaⅡ K LINE PROFILES OF THE FLARES ON MARCH 9 AND 14,1989[J]. Publications of the Yunnan Observatory, 1990, (4): 38-41.

AR5395:OBSERVATIONS ON THE ASYMMETRIES OF THE Hα AND CaⅡ K LINE PROFILES OF THE FLARES ON MARCH 9 AND 14,1989

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The most powerful method to diagnose the velocity field in solar flare atmosphere isspectral analyses. That is to analyse the asymmetry and the Doppler shift of flare spectralline profiles.

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AR5395:OBSERVATIONS ON THE ASYMMETRIES OF THE Hα AND CaⅡ K LINE PROFILES OF THE FLARES ON MARCH 9 AND 14,1989

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