Triggering of whistler mode emissions by the band‐limited impulse (BLI) Associated with amplified Vlf signals from Siple Station, Antarctica
2000
At termination of an amplified and saturated (B sat ) Vlf pulse from Siple Station, Antarctica,a band-limited (50-500 Hz range) impulse (BLI) is generated which in turn triggers a narrowband emission, of about the same amplitude, that starts at about 50-150 Hz above the frequency of B sat , called the positive frequency offset (PFO). The BLI creates the PFO by reducing the parallel velocities of existing phase-bunched cyclotron resonant electrons that form the source currents (J⊥) of the stimulated radiation. The PFO is proportional to the magnetic field intensity B BLI of the BLI. Since B BLI ≃ B sat the PFO then becomes a measure of the saturated field B sat . An example for L = 4 and a pitch angle of 60°, gives B sat ≅ 5pT, in good agreement with previous estimates of B sat .
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