Statistics – Computation
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982m%26p....26..227k&link_type=abstract
Moon and the Planets, vol. 26, Apr. 1982, p. 227-233.
Statistics
Computation
2
Earth Magnetosphere, Electron Energy, Hiss, Jupiter Atmosphere, Very Low Frequencies, Cerenkov Radiation, Resonance
Scientific paper
Computation of the Jovian magnetosphere's VLF hiss-generating particle energy under longitudinal and transverse resonance conditions shows that the minimum energy required for electron generation of VLF hiss under the former condition is 100 eV-1keV at 2-10 kHz, while the corresponding transverse resonance condition energy range for the same frequencies is 8 keV-40 keV. Also computed is the average power radiated by the Cerenkov process in the Jupiter magnetosphere at L values of 5.6 Rj, at the 5 kHz wave frequency, for the cases 10 eV, 100 eV, and 1 keV electron energy.
Ahmad Mushfiq
Khosa P. N.
Lalmani
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