Dependence of the spectrum of Pc 3–4 pulsations on the interplanetary magnetic field
- 1 May 1984
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 89 (A5) , 2770-2780
- https://doi.org/10.1029/ja089ia05p02770
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- The electromagnetic ion beam instability upstream of the Earth's bow shockJournal of Geophysical Research, 1981
- Geomagnetic pulsation signals and hourly distributions of IMF orientationJournal of Geophysical Research, 1979
- IMF orientation, solar wind velocity, and Pc 3‐4 signals: A joint distributionJournal of Geophysical Research, 1979
- Interplanetary magnetic field conditions associated with synchronous orbit observations of Pc 3 magnetic pulsationsJournal of Geophysical Research, 1977
- A contribution to ULF activity in the Pc 3-4 range correlated with IMF radial orientationJournal of Geophysical Research, 1977
- Pc 3, 4 activity and interplanetary field orientationJournal of Geophysical Research, 1976
- Magnetic fields of the magnetosheathReviews of Geophysics, 1976
- A model for generation of bow-shock-associated upstream wavesJournal of Geophysical Research, 1975
- A theory of long-period magnetic pulsations: 1. Steady state excitation of field line resonanceJournal of Geophysical Research, 1974
- Bow shock associated waves observed in the far upstream interplanetary mediumJournal of Geophysical Research, 1969