SPECTRUM OF THE INTERPLANETARY PLASMA TURBULENCE AT A DISTANCE FROM THE SUN GREATER THAN 1 AU

SPECTRUM OF THE INTERPLANETARY PLASMA TURBULENCE AT A DISTANCE FROM THE SUN GREATER THAN 1 AU

Purpose: Making analysis of variations of fast and slow solarwind parameters at distances from the Sun of about 1 AU and more. Design/methodology/approach: The method of Feynman pathintegrals is applied to calculate the temporal spectra and dispersion dependences of the drift velocity of interpla...

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Bibliographic Details
Main Authors: M. R. Olyak, N. N. Kalinichenko, A. A. Konovalenko, A. I. Brazhenko, I. N. Bubnov
Format: Article
Language:English
Published: National Academy of Sciences of Ukraine, Institute of Radio Astronomy 2016-12-01
Series:Radio Physics and Radio Astronomy
Subjects:
interplanetary scintillation
fast and slow solar wind
three-dimensional spatial spectrum of electron density fluctuations
Online Access:http://rpra-journal.org.ua/index.php/ra/article/view/1248/pdf

Internet

http://rpra-journal.org.ua/index.php/ra/article/view/1248/pdf

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