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- W2120553917 abstract "Soft X-rays irradiation of the solar atmosphere during solar flares generates photoelectrons which have an anisotropic velocity distribution. Using a 1-D test particle code, the anisotropy of the photoelectrons velocity distribution is de- rived, and the maximum degree of linear polarization in the hydrogen H and H lines that photoelectrons could generate by impact is estimated. Over a band pass of 0.75 and 0.5 ˚ A, the net polarization degree expected in both lines is predicted not to exceed 0.2%. Therefore, soft X-ray irradiation cannot explain the one order of magnitude higher degree of linear polarization observed in solar flares." @default.
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- W2120553917 date "1999-01-01" @default.
- W2120553917 modified "2023-09-24" @default.
- W2120553917 title "VELOCITY DISTRIBUTION FUNCTION ANISOTROPY OF SOFT X-RAY GENERATED PHOTOELECTRONS AND RESULTING HALPHA POLARIZATION IN SOLAR FLARES" @default.
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