Solar irradiance change and special longitudes due to r-modes

Details Solar irradiance change and special longitudes due to r-modes Solar irradiance change and special longitudes due to r-modes

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sci...235.1631w&link_type=abstract

Science (ISSN 0036-8075), vol. 235, March 27, 1987, p. 1631-1633.

Other

27

Planetary Waves, Solar Activity, Solar Longitude, Solar Radiation, Solar Cycles, Solar Oscillations, Solar Rotation

Scientific paper

Sluggish global oscillations, having a periodicity of months and trapped in the sun's convection zone, modulate the amount of energy reaching earth and seem to impose some large-scale order on the distribution of solar surface features. These recently recognized oscillations (r-modes) increase the predictability of solar changes and may improve understanding of rotation and variability in other stars. Most of the 13 periodicities ranging from 13 to 85 days that are caused by r-modes can be detected in Nimbus 7 observations of solar irradiance during 3 years at solar maximum. These modes may also bear on the classical question of persistent longitudes of high solar activity.

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