Properties of the magnetospheric hot plasma distribution deduced from whistler mode wave injection at 2400 Hz: Ground‐based detection of azimuthal structure in magnetospheric hot plasmas

Author:

Sonwalkar Vikas S.,Carpenter D. L.,Helliwell R. A.,Walt M.,Inan U. S.,Caudle D. L.,Ikeda M.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference39 articles.

1. Whistler duct properties deduced from VLF observations made with the Ogo 3 satellite near the magnetic equator

2. Protonospheric-ionospheric modeling of VLF ducts

3. Banded electron structures in the plasmasphere

4. Carlson C. R. Simulation and modeling of whistler mode wave growth through cyclotron resonance with energetic electrons in the magnetosphere Ph.D. thesis Stanford Univ. Stanford Calif. 1987.

5. Variable frequency VLF signals in the magnetosphere: Associated phenomena and plasma diagnostics

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