The power spectrum of interplanetary Alfvénic fluctuations: Derivation of the governing equation and its solution
- 1 November 1984
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 89 (A11) , 9695-9702
- https://doi.org/10.1029/ja089ia11p09695
Abstract
No abstract availableKeywords
This publication has 28 references indexed in Scilit:
- Heliospheric magnetic fields and plasmasReviews of Geophysics, 1983
- Statistical properties of MHD fluctuations associated with high-speed streams from Helios-2 observationsSolar Physics, 1982
- Radial evolution of power spectra of interplanetary Alfvénic turbulenceJournal of Geophysical Research, 1982
- Statistical properties of low‐frequency magnetic field fluctuations in the solar wind from 0.29 to 1.0 AU during solar minimum conditions: HELIOS 1 and HELIOS 2Journal of Geophysical Research, 1982
- On the polarization state of hydromagnetic fluctuations in the solar windJournal of Geophysical Research, 1981
- Magnetic fields, plasmas, and coronal holes: The inner solar systemSpace Science Reviews, 1979
- Heliocentric distance dependence of the interplanetary magnetic fieldReviews of Geophysics, 1978
- Large-amplitude hydromagnetic wavesJournal of Geophysical Research, 1974
- Large-amplitude Alfvén waves in the interplanetary medium, 2Journal of Geophysical Research, 1971
- Turbulence, Viscosity, and Dissipation in the Solar-Wind PlasmaThe Astrophysical Journal, 1968