On the amplitude modulation of low-degree solar p-modes

Details On the amplitude modulation of low-degree solar p-modes On the amplitude modulation of low-degree solar p-modes

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...286..635g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 286, no. 2, p. 635-638

Astronomy and Astrophysics

Astrophysics

Amplitude Modulation, Compression Waves, P Waves, Solar Activity, Solar Atmosphere, Solar Oscillations, Solar Spectra, Spectral Energy Distribution, Statistical Analysis

Scientific paper

The amplitude modulation of low-degree solar p-modes obtained from the analysis of daily data observed at International Research on the Interior of the Sun (IRIS) network station at Kumbel (Uzbekistan) is discussed using the statistical approach of Gabriel (1993). It is found that the dispersion in peak energy reflects mainly the length of the daily observations. We conclude that there is no contradiction between observations and theory and if observational results are taken at face value, we can rule out some type of mode correlations.

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