On the origin of the 1/f spectrum of fluctuations in the solar wind

Details On the origin of the 1/f spectrum of fluctuations in the solar wind On the origin of the 1/f spectrum of fluctuations in the solar wind

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..225r&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 225

Physics

2

Particle Emission, Solar Wind, Interplanetary Magnetic Fields

Scientific paper

The origin of the 1/f low-frequency spectrum of fluctuations observed in the solar wind is discussed. It is suggested that this spectrum arises due to sampling random perturbations produced at the Sun. The perturbation process is characterized by a power-law distribution. It is pointed out that, due to solar rotation, the sampling is equivalent to scanning across different size scales on the Sun. The limits of the spectrum found from the observations are used to estimate the characteristic scales on the Sun, the scales related to the origin of the solar wind.

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