Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2835
Title: Amplitude of solar wind density turbulence from 10 to 45 R⊙
Authors: Raja, K. Sasikumar
INGALE, MADHUSUDAN
Ramesh, V
SUBRAMANIAN, PRASAD
Manoharan, P. K.
Janardhan, P.
Dept. of Physics
Keywords: Occultation
Turbulence
Solar corona
Solar wind density
Fluctuations
Solar cycle
2016
Issue Date: Dec-2016
Publisher: American Geophysical Union
Citation: Journal of Geophysical Research: Space Physics, 121(12), 605-619.
Abstract: We report on the amplitude of the density turbulence spectrum ( urn:x-wiley:jgra:media:jgra53108:jgra53108-math-0001) and the density modulation index (δN/N) in the solar wind between 10 and 45R⊙. We derive these quantities using a structure function that is observationally constrained by occultation observations of the Crab nebula made in 2011 and 2013 and similar observations published earlier. We use the most general form of the structure function, together with currently used prescriptions for the inner/dissipation scale of the turbulence spectrum. Our work yields a comprehensive picture (a) of the manner in which urn:x-wiley:jgra:media:jgra53108:jgra53108-math-0002 and δN/N vary with heliocentric distance in the solar wind and (b) of the solar cycle dependence of these quantities.
URI: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2835
https://doi.org/10.1002/2016JA023254
ISSN: 2169-9402
2169-9402
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