Dynamics of solar filaments. V - Oscillations in the H-alpha and 1548 A C IV lines

Details Dynamics of solar filaments. V - Oscillations in the H-alpha and 1548 A C IV lines Dynamics of solar filaments. V - Oscillations in the H-alpha and 1548 A C IV lines

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...172..316m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 172, no. 1-2, Jan. 1987, p. 316-322.

Astronomy and Astrophysics

Astrophysics

13

Line Spectra, Mass Transfer, Solar Oscillations, Solar Prominences, Ultraviolet Spectra, Astronomical Maps, Carbon, Energy Spectra, H Alpha Line, Solar Maximum Mission

Scientific paper

Using the Multichannel Subtractive Double Pass Spectrograph operating in the Meudon solar tower and the Ultraviolet Spectrometer and Polarimeter aboard the Solar Maximum Mission satellite, the authors analyze by Fourier transform technique time sequence observations of filaments in both the Hα line and in the 1548 Å C IV line. The Hα data confirm previous findings that there are no oscillations at the location of the filament in the observed range 1 - 10 mHz. In the C IV line the authors observe power in some parts of the filament where a steady velocity gradient is present, e.g. in the footpoints. The energy is probably due to convective motions rather than pressure oscillations.

Affiliated with

Also associated with

No associations

Rating

Dynamics of solar filaments. V - Oscillations in the H-alpha and 1548 A C IV lines does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamics of solar filaments. V - Oscillations in the H-alpha and 1548 A C IV lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of solar filaments. V - Oscillations in the H-alpha and 1548 A C IV lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1621510