Dynamics of a Quiescent Solar Prominence Observed with the SUMER/SOHO Instrument

Details Dynamics of a Quiescent Solar Prominence Observed with the SUMER/SOHO Instrument Dynamics of a Quiescent Solar Prominence Observed with the SUMER/SOHO Instrument

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..199..133b&link_type=abstract

Solar Physics, v. 199, Issue 1, p. 133-143 (2001).

Physics

8

Scientific paper

We present the results obtained from analyzing SUMER/SOHO observational data of a quiescent solar prominence. The studied prominence is made of complex structures. From the 1-hr data set, we derive characteristic frequencies in terms of intensity and velocity oscillations, as measured in 4 transition-region lines. The presence of different types of frequencies is detected: chromospheric oscillations and intermediate periods (6 min to 12 min). This result suggests that these oscillations are transmitted by the magnetic fields from the chromosphere to the transition region.

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