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3. Spectral diagnoses

The prominence was scanned with tex2html_wrap_inline834 line from the left to the right of the filtergrams of Fig. 1 (click here), and the slit was parallel to the left edge of each filtergram. The scanning time was 0927UT to 0930UT. Combining the tex2html_wrap_inline834 spectra and tex2html_wrap_inline832 filtergrams, we can infer that the materials in the left leg of the eruptive prominence spiraled to rise. This is consistent with the results obtained in section two. The tex2html_wrap_inline834 spectra obtained were measured with the PDS microdensitometer at the Purple Mountain Observatory. Comparing the spectra with the tex2html_wrap_inline832 filtergrams, we can locate the position of each tex2html_wrap_inline834 line in the filtergrams of the prominence. After calculating the center-of-gravity position (tex2html_wrap_inline886) of each chosen line profile and then the Doppler shift tex2html_wrap_inline888 (tex2html_wrap_inline890, tex2html_wrap_inline892), we obtained the velocity along the line of sight tex2html_wrap_inline894 (tex2html_wrap_inline896). Figure 4 (click here) gives the distribution of the line-of-sight velocity, which indicates that the velocity increased from the bottom of the left leg to the top. After the materials in the left leg reached the climax, those dropped out in succession and did not spiral. Figure 4 (click here)b summarises the configuration of the velocity distribution. The materials are usually frozen in the magnetic field of a prominence, and they move mostly along the magnetic lines. So we think of the magnetic field of the prominence helical, stretched primarily along the axis, and tied to the photosphere only at the end of the prominence. There is growing evidence that filaments (or prominences) emerge from the photosphere already twisted (Rust & Kumar 1994; Yang et al. 1988; Liggett & Zirin 1984; Vrsnak et al. 1991). The prominence motion shown in Fig. 4 (click here)b may be called "right-hand screw" when it is viewed by a hypothetical observer in the chromosphere. Rust & Kumar (1994) infer that the magnetic fields of prominences are twisted in a systematic way: right-hand helices predominate in the south and left-hand helices predominate in the north. The result obtained by spectral analyses confirms their inference. The velocity increased perhaps because (1) the angular velocity increased from the bottom to the top due to the release of the torsion of the prominence; (2) the angular velocity may be constant, but the radius of the leg increased from the bottom to the top.

  figure289
Figure 4: a) Distribution of the velocity (in km/s) along the line of sight. b) Sketch for explanation of the velocity distribution. The arrow shows the direction of the material motion


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