Subionospheric VLF observations of transmitter-induced precipitation of inner radiation belt electrons

被引:43
|
作者
Inan, U. S. [1 ]
Golkowski, M.
Casey, M. K.
Moore, R. C.
Peter, W.
Kulkarni, P.
Kossey, P.
Kennedy, E.
Meth, S.
Smit, P.
机构
[1] Stanford Univ, Space Telecommun & Radiosci Lab, Stanford, CA 94305 USA
[2] USN, Res Lab, Washington, DC 20375 USA
[3] USAF, Res Lab, Bedford, MA 01731 USA
[4] Def Adv Res Projects Agcy, Arlington, VA 22203 USA
关键词
D O I
10.1029/2006GL028494
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Ionospheric effects of energetic electron precipitation induced by controlled injection of VLF signals from a ground based transmitter are observed via subionospheric VLF remote sensing. The 21.4 kHz NPM transmitter in Lualualei, Hawaii is keyed ON-OFF in 30 minute periodic sequences. The same periodicity is observed in the amplitude and phase of the sub ionospherically propagating signals of the 24.8 kHz NLK (Jim Creek, Washington) and 25.2 kHz NLM (LaMoure, North Dakota) transmitters measured at Midway Island. Periodic perturbations of the NLK signal observed at Palmer, Antarctica suggest that energetic electrons scattered at longitudes of NPM continue to be precipitated into the atmosphere as they drift toward the South Atlantic Anomaly. Utilizing a model of the magnetospheric wave-particle interaction, ionospheric energy deposition, and subionospheric VLF propagation, the precipitated energy flux induced by the NPM transmitter is estimated to peak at L similar to 2 and similar to 1.6 X 10(-4) ergs s(-1) cm(-2).
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页数:6
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