High-frequency oscillations in the corona observed at the 1983 eclipse

Details High-frequency oscillations in the corona observed at the 1983 eclipse High-frequency oscillations in the corona observed at the 1983 eclipse

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..109..365p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 109, no. 2, 1987, p. 365-372. Research supported by the National Georaphic Society and Will

Physics

Optics

38

Coronal Loops, High Frequencies, Solar Corona, Solar Eclipses, Solar Oscillations, Atmospheric Effects, Fiber Optics, Fourier Transformation, Indonesia, Magnetohydrodynamic Waves, Phase Transformations

Scientific paper

The authors detected excess oscillatory power at 0.25 - 2.0 Hz in a coronal loop in the 1983 Indonesian total solar eclipse. In this second-generation experiment enlarging upon the work of Pasachoff and Landman (1984), they observed in two frequency channels, one coronal and one continuum, to monitor atmospheric and instrumental effects. They briefly discuss the effects of an oscillation near 1 Hz on the coronal heating problem.

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