Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-06-22T23:38:09.014Z Has data issue: false hasContentIssue false
  • English
  • Français

3D Kinematic Evolution of Erupting Filaments

Published online by Cambridge University Press:  27 June 2012

M. Faurobert ,
C. Fang ,
T. Corbard ,
T. Li ,
J. Zhang ,
Y. Zhang  and
S. Yang
T. Li
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
J. Zhang
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Y. Zhang
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
S. Yang
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Get access

Abstract

We reconstruct the three-dimensional geometry of erupting filaments using observations from different viewpoints. True kinematic evolution of different locations along the main bodies of filaments is investigated. For the erupting filament on 2009 September 26, the highest point is the fastest in the first half hour, and then the points at the low-latitude leg of the filament become the fastest. However, for the event on 2010 August 1, the highest location always has the largest velocity and acceleration during the eruption process. The propagation of EUV enhancements at the endpoints of the erupting filament is observed clearly, which is attributed to the successive down-flows along the different groups of thread-like structures of the filament. Both the two filaments show non-radial eruptions and move towards low-latitude region. Their latitudinal variation is greater than the longitudinal.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 55: 4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges , 2012 , pp. 179 - 184
Copyright
© EAS, EDP Sciences 2012

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Howard, R.A., et al., 2008, Space Sci. Rev., 136, 67 CrossRef
Kaiser, M.L., Kucera, T.A., Davila, J.M., et al., 2008, Space Sci. Rev., 136, 5 CrossRef
Kliem, B., Titov, V.S., & Török, T., 2004, ApJ, 413, L23
Li, T., Zhang, J., Zhang, Y., & Yang, S., 2011, ApJ, 739, 43 CrossRef
Li, T., Zhang, J., Zhao, H., & Yang, S., 2010, ApJ, 720, 144 CrossRef
Scherrer, P.H., Schou, J., Bush, R.I., et al., 2011, Sol. Phys., DOI : 10.1007/s11207-011-9834-2
Schmieder, B., Démoulin, P., Aulanier, G., & Golub, L., 1996, ApJ, 467, 881 CrossRef
Wang, Y., Muglach, K., & Kliem, B., 2009, ApJ, 699, 133 CrossRef